proton form factors
DESCRIPTION
Proton Form Factors. Q 2 ≤ 1 GeV 2. F1. F2. Over a period of time lasting at least 2000 years, Man has puzzled over and sought an understanding of the composition of matter…. Electromagnetic Hadron Form Factors in Space and Time-like regions. Egle Tomasi-Gustafsson Saclay, France. - PowerPoint PPT PresentationTRANSCRIPT
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 1
Proton Form Factors
QQ22lele1 GeV1 GeV22
F2F2
F1F1
Over a period of time lasting at least 2000 years Man has puzzled over and sought
an understanding of the composition of matterhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 2
Electromagnetic Hadron Form Factors Electromagnetic Hadron Form Factors in Space and Time-like regions in Space and Time-like regions
Egle Tomasi-GustafssonSaclay France
JLab May 2 2008
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 3
PLANPLANExperimental view
ndash space-like (ep-scattering)ndash time-like (e+e- or pp annihilation)
Model Independent Statementsndash Symmetry properties of fundamental interactionsndash Kinematical constraints
Models and lsquoexactrsquo calculations Radiative corrections
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 4
Hadron Electromagnetic Form factorsHadron Electromagnetic Form factors
ndash Characterize the internal structure of a particle
( point-like)
ndash Elastic form factors contain information on the
hadron ground state
ndash In a P- and T-invariant theory the EM structure of a
particle of spin S is defined by 2S+1 form factors
ndash Neutron and proton form factors are different
ndash Deuteron 2 structure functions but 3 form factors
ndash Playground for theory and experiment
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 5
Space-like and time-like regionsSpace-like and time-like regions
bullFFs are analytical functionsbullIn framework of one photon exchange FFs are functions of the
momentum transfer squared of the virtual photon t = q2 = -Q2
ScatterinScatteringg
e- + h =gt e- + h e+ + e- =gt h + h
_
AnnihilationAnnihilation
_
Form factors are real in the space-like region complex in the time-like region
tlt0 tgt0
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 6
Crossing SymmetryCrossing Symmetry
Scattering and annihilation channels
- Described by the same amplitude
- function of two kinematical variables s and t
p2 rarr ndash p2
k2 rarr ndash k2
- which scan different kinematical regions
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 7
Proton Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 8
Proton Form Factors Ratio
POLARIZATION ExpJlab E93-027 E99-007 SpokepersonsCh Perdrisat V Punjabi M Jones E Brash M Jones et al Phys Rev Lett 841398 (2000)O Gayou et al Phys Rev Lett 88092301 (2002)V Punjabi et al Phys Rev C 71 055202 (2005)
Linear deviation from dipole GEpGMp
Jlab Super RosenbluthIA Qattan et alPRL 94 142301 (2005)
Jlab E04-108019 NOW running
SLAC RosenbluthL Andivahis PRD505491 (1994)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 9
The Rosenbluth separation (1950)The Rosenbluth separation (1950)
bullElastic ep cross section (1 exchange)
bull point-like particle Mott
Linearity of the reduced cross section
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 10
The Rosenbluth separation The Rosenbluth separation
The dynamics is contained in FFs
Q2
The kinematics energies angles
The reaction mechanism
Holds for 1 exchange only
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 11
Rosenbluth separationRosenbluth separation
=05=02
=08
Contribution of the electric term
hellipto be compared to the absolute value of the error on and to the size and dependence of RC
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 12
The polarization induces a term in the cross section proportional to GE GM
Polarized beam and target or
polarized beam and recoil proton polarization
The polarization method (1967)The polarization method (1967)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 13
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 14
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 2
Electromagnetic Hadron Form Factors Electromagnetic Hadron Form Factors in Space and Time-like regions in Space and Time-like regions
Egle Tomasi-GustafssonSaclay France
JLab May 2 2008
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 3
PLANPLANExperimental view
ndash space-like (ep-scattering)ndash time-like (e+e- or pp annihilation)
Model Independent Statementsndash Symmetry properties of fundamental interactionsndash Kinematical constraints
Models and lsquoexactrsquo calculations Radiative corrections
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 4
Hadron Electromagnetic Form factorsHadron Electromagnetic Form factors
ndash Characterize the internal structure of a particle
( point-like)
ndash Elastic form factors contain information on the
hadron ground state
ndash In a P- and T-invariant theory the EM structure of a
particle of spin S is defined by 2S+1 form factors
ndash Neutron and proton form factors are different
ndash Deuteron 2 structure functions but 3 form factors
ndash Playground for theory and experiment
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 5
Space-like and time-like regionsSpace-like and time-like regions
bullFFs are analytical functionsbullIn framework of one photon exchange FFs are functions of the
momentum transfer squared of the virtual photon t = q2 = -Q2
ScatterinScatteringg
e- + h =gt e- + h e+ + e- =gt h + h
_
AnnihilationAnnihilation
_
Form factors are real in the space-like region complex in the time-like region
tlt0 tgt0
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 6
Crossing SymmetryCrossing Symmetry
Scattering and annihilation channels
- Described by the same amplitude
- function of two kinematical variables s and t
p2 rarr ndash p2
k2 rarr ndash k2
- which scan different kinematical regions
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 7
Proton Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 8
Proton Form Factors Ratio
POLARIZATION ExpJlab E93-027 E99-007 SpokepersonsCh Perdrisat V Punjabi M Jones E Brash M Jones et al Phys Rev Lett 841398 (2000)O Gayou et al Phys Rev Lett 88092301 (2002)V Punjabi et al Phys Rev C 71 055202 (2005)
Linear deviation from dipole GEpGMp
Jlab Super RosenbluthIA Qattan et alPRL 94 142301 (2005)
Jlab E04-108019 NOW running
SLAC RosenbluthL Andivahis PRD505491 (1994)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 9
The Rosenbluth separation (1950)The Rosenbluth separation (1950)
bullElastic ep cross section (1 exchange)
bull point-like particle Mott
Linearity of the reduced cross section
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 10
The Rosenbluth separation The Rosenbluth separation
The dynamics is contained in FFs
Q2
The kinematics energies angles
The reaction mechanism
Holds for 1 exchange only
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 11
Rosenbluth separationRosenbluth separation
=05=02
=08
Contribution of the electric term
hellipto be compared to the absolute value of the error on and to the size and dependence of RC
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 12
The polarization induces a term in the cross section proportional to GE GM
Polarized beam and target or
polarized beam and recoil proton polarization
The polarization method (1967)The polarization method (1967)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 13
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 14
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 3
PLANPLANExperimental view
ndash space-like (ep-scattering)ndash time-like (e+e- or pp annihilation)
Model Independent Statementsndash Symmetry properties of fundamental interactionsndash Kinematical constraints
Models and lsquoexactrsquo calculations Radiative corrections
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 4
Hadron Electromagnetic Form factorsHadron Electromagnetic Form factors
ndash Characterize the internal structure of a particle
( point-like)
ndash Elastic form factors contain information on the
hadron ground state
ndash In a P- and T-invariant theory the EM structure of a
particle of spin S is defined by 2S+1 form factors
ndash Neutron and proton form factors are different
ndash Deuteron 2 structure functions but 3 form factors
ndash Playground for theory and experiment
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 5
Space-like and time-like regionsSpace-like and time-like regions
bullFFs are analytical functionsbullIn framework of one photon exchange FFs are functions of the
momentum transfer squared of the virtual photon t = q2 = -Q2
ScatterinScatteringg
e- + h =gt e- + h e+ + e- =gt h + h
_
AnnihilationAnnihilation
_
Form factors are real in the space-like region complex in the time-like region
tlt0 tgt0
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 6
Crossing SymmetryCrossing Symmetry
Scattering and annihilation channels
- Described by the same amplitude
- function of two kinematical variables s and t
p2 rarr ndash p2
k2 rarr ndash k2
- which scan different kinematical regions
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 7
Proton Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 8
Proton Form Factors Ratio
POLARIZATION ExpJlab E93-027 E99-007 SpokepersonsCh Perdrisat V Punjabi M Jones E Brash M Jones et al Phys Rev Lett 841398 (2000)O Gayou et al Phys Rev Lett 88092301 (2002)V Punjabi et al Phys Rev C 71 055202 (2005)
Linear deviation from dipole GEpGMp
Jlab Super RosenbluthIA Qattan et alPRL 94 142301 (2005)
Jlab E04-108019 NOW running
SLAC RosenbluthL Andivahis PRD505491 (1994)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 9
The Rosenbluth separation (1950)The Rosenbluth separation (1950)
bullElastic ep cross section (1 exchange)
bull point-like particle Mott
Linearity of the reduced cross section
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 10
The Rosenbluth separation The Rosenbluth separation
The dynamics is contained in FFs
Q2
The kinematics energies angles
The reaction mechanism
Holds for 1 exchange only
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 11
Rosenbluth separationRosenbluth separation
=05=02
=08
Contribution of the electric term
hellipto be compared to the absolute value of the error on and to the size and dependence of RC
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 12
The polarization induces a term in the cross section proportional to GE GM
Polarized beam and target or
polarized beam and recoil proton polarization
The polarization method (1967)The polarization method (1967)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 13
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 14
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 4
Hadron Electromagnetic Form factorsHadron Electromagnetic Form factors
ndash Characterize the internal structure of a particle
( point-like)
ndash Elastic form factors contain information on the
hadron ground state
ndash In a P- and T-invariant theory the EM structure of a
particle of spin S is defined by 2S+1 form factors
ndash Neutron and proton form factors are different
ndash Deuteron 2 structure functions but 3 form factors
ndash Playground for theory and experiment
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 5
Space-like and time-like regionsSpace-like and time-like regions
bullFFs are analytical functionsbullIn framework of one photon exchange FFs are functions of the
momentum transfer squared of the virtual photon t = q2 = -Q2
ScatterinScatteringg
e- + h =gt e- + h e+ + e- =gt h + h
_
AnnihilationAnnihilation
_
Form factors are real in the space-like region complex in the time-like region
tlt0 tgt0
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 6
Crossing SymmetryCrossing Symmetry
Scattering and annihilation channels
- Described by the same amplitude
- function of two kinematical variables s and t
p2 rarr ndash p2
k2 rarr ndash k2
- which scan different kinematical regions
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 7
Proton Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 8
Proton Form Factors Ratio
POLARIZATION ExpJlab E93-027 E99-007 SpokepersonsCh Perdrisat V Punjabi M Jones E Brash M Jones et al Phys Rev Lett 841398 (2000)O Gayou et al Phys Rev Lett 88092301 (2002)V Punjabi et al Phys Rev C 71 055202 (2005)
Linear deviation from dipole GEpGMp
Jlab Super RosenbluthIA Qattan et alPRL 94 142301 (2005)
Jlab E04-108019 NOW running
SLAC RosenbluthL Andivahis PRD505491 (1994)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 9
The Rosenbluth separation (1950)The Rosenbluth separation (1950)
bullElastic ep cross section (1 exchange)
bull point-like particle Mott
Linearity of the reduced cross section
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 10
The Rosenbluth separation The Rosenbluth separation
The dynamics is contained in FFs
Q2
The kinematics energies angles
The reaction mechanism
Holds for 1 exchange only
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 11
Rosenbluth separationRosenbluth separation
=05=02
=08
Contribution of the electric term
hellipto be compared to the absolute value of the error on and to the size and dependence of RC
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 12
The polarization induces a term in the cross section proportional to GE GM
Polarized beam and target or
polarized beam and recoil proton polarization
The polarization method (1967)The polarization method (1967)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 13
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 14
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 5
Space-like and time-like regionsSpace-like and time-like regions
bullFFs are analytical functionsbullIn framework of one photon exchange FFs are functions of the
momentum transfer squared of the virtual photon t = q2 = -Q2
ScatterinScatteringg
e- + h =gt e- + h e+ + e- =gt h + h
_
AnnihilationAnnihilation
_
Form factors are real in the space-like region complex in the time-like region
tlt0 tgt0
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 6
Crossing SymmetryCrossing Symmetry
Scattering and annihilation channels
- Described by the same amplitude
- function of two kinematical variables s and t
p2 rarr ndash p2
k2 rarr ndash k2
- which scan different kinematical regions
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 7
Proton Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 8
Proton Form Factors Ratio
POLARIZATION ExpJlab E93-027 E99-007 SpokepersonsCh Perdrisat V Punjabi M Jones E Brash M Jones et al Phys Rev Lett 841398 (2000)O Gayou et al Phys Rev Lett 88092301 (2002)V Punjabi et al Phys Rev C 71 055202 (2005)
Linear deviation from dipole GEpGMp
Jlab Super RosenbluthIA Qattan et alPRL 94 142301 (2005)
Jlab E04-108019 NOW running
SLAC RosenbluthL Andivahis PRD505491 (1994)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 9
The Rosenbluth separation (1950)The Rosenbluth separation (1950)
bullElastic ep cross section (1 exchange)
bull point-like particle Mott
Linearity of the reduced cross section
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 10
The Rosenbluth separation The Rosenbluth separation
The dynamics is contained in FFs
Q2
The kinematics energies angles
The reaction mechanism
Holds for 1 exchange only
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 11
Rosenbluth separationRosenbluth separation
=05=02
=08
Contribution of the electric term
hellipto be compared to the absolute value of the error on and to the size and dependence of RC
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 12
The polarization induces a term in the cross section proportional to GE GM
Polarized beam and target or
polarized beam and recoil proton polarization
The polarization method (1967)The polarization method (1967)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 13
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 14
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 6
Crossing SymmetryCrossing Symmetry
Scattering and annihilation channels
- Described by the same amplitude
- function of two kinematical variables s and t
p2 rarr ndash p2
k2 rarr ndash k2
- which scan different kinematical regions
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 7
Proton Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 8
Proton Form Factors Ratio
POLARIZATION ExpJlab E93-027 E99-007 SpokepersonsCh Perdrisat V Punjabi M Jones E Brash M Jones et al Phys Rev Lett 841398 (2000)O Gayou et al Phys Rev Lett 88092301 (2002)V Punjabi et al Phys Rev C 71 055202 (2005)
Linear deviation from dipole GEpGMp
Jlab Super RosenbluthIA Qattan et alPRL 94 142301 (2005)
Jlab E04-108019 NOW running
SLAC RosenbluthL Andivahis PRD505491 (1994)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 9
The Rosenbluth separation (1950)The Rosenbluth separation (1950)
bullElastic ep cross section (1 exchange)
bull point-like particle Mott
Linearity of the reduced cross section
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 10
The Rosenbluth separation The Rosenbluth separation
The dynamics is contained in FFs
Q2
The kinematics energies angles
The reaction mechanism
Holds for 1 exchange only
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 11
Rosenbluth separationRosenbluth separation
=05=02
=08
Contribution of the electric term
hellipto be compared to the absolute value of the error on and to the size and dependence of RC
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 12
The polarization induces a term in the cross section proportional to GE GM
Polarized beam and target or
polarized beam and recoil proton polarization
The polarization method (1967)The polarization method (1967)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 13
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 14
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 7
Proton Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 8
Proton Form Factors Ratio
POLARIZATION ExpJlab E93-027 E99-007 SpokepersonsCh Perdrisat V Punjabi M Jones E Brash M Jones et al Phys Rev Lett 841398 (2000)O Gayou et al Phys Rev Lett 88092301 (2002)V Punjabi et al Phys Rev C 71 055202 (2005)
Linear deviation from dipole GEpGMp
Jlab Super RosenbluthIA Qattan et alPRL 94 142301 (2005)
Jlab E04-108019 NOW running
SLAC RosenbluthL Andivahis PRD505491 (1994)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 9
The Rosenbluth separation (1950)The Rosenbluth separation (1950)
bullElastic ep cross section (1 exchange)
bull point-like particle Mott
Linearity of the reduced cross section
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 10
The Rosenbluth separation The Rosenbluth separation
The dynamics is contained in FFs
Q2
The kinematics energies angles
The reaction mechanism
Holds for 1 exchange only
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 11
Rosenbluth separationRosenbluth separation
=05=02
=08
Contribution of the electric term
hellipto be compared to the absolute value of the error on and to the size and dependence of RC
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 12
The polarization induces a term in the cross section proportional to GE GM
Polarized beam and target or
polarized beam and recoil proton polarization
The polarization method (1967)The polarization method (1967)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 13
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 14
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 8
Proton Form Factors Ratio
POLARIZATION ExpJlab E93-027 E99-007 SpokepersonsCh Perdrisat V Punjabi M Jones E Brash M Jones et al Phys Rev Lett 841398 (2000)O Gayou et al Phys Rev Lett 88092301 (2002)V Punjabi et al Phys Rev C 71 055202 (2005)
Linear deviation from dipole GEpGMp
Jlab Super RosenbluthIA Qattan et alPRL 94 142301 (2005)
Jlab E04-108019 NOW running
SLAC RosenbluthL Andivahis PRD505491 (1994)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 9
The Rosenbluth separation (1950)The Rosenbluth separation (1950)
bullElastic ep cross section (1 exchange)
bull point-like particle Mott
Linearity of the reduced cross section
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 10
The Rosenbluth separation The Rosenbluth separation
The dynamics is contained in FFs
Q2
The kinematics energies angles
The reaction mechanism
Holds for 1 exchange only
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 11
Rosenbluth separationRosenbluth separation
=05=02
=08
Contribution of the electric term
hellipto be compared to the absolute value of the error on and to the size and dependence of RC
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 12
The polarization induces a term in the cross section proportional to GE GM
Polarized beam and target or
polarized beam and recoil proton polarization
The polarization method (1967)The polarization method (1967)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 13
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 14
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 9
The Rosenbluth separation (1950)The Rosenbluth separation (1950)
bullElastic ep cross section (1 exchange)
bull point-like particle Mott
Linearity of the reduced cross section
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 10
The Rosenbluth separation The Rosenbluth separation
The dynamics is contained in FFs
Q2
The kinematics energies angles
The reaction mechanism
Holds for 1 exchange only
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 11
Rosenbluth separationRosenbluth separation
=05=02
=08
Contribution of the electric term
hellipto be compared to the absolute value of the error on and to the size and dependence of RC
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 12
The polarization induces a term in the cross section proportional to GE GM
Polarized beam and target or
polarized beam and recoil proton polarization
The polarization method (1967)The polarization method (1967)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 13
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 14
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 10
The Rosenbluth separation The Rosenbluth separation
The dynamics is contained in FFs
Q2
The kinematics energies angles
The reaction mechanism
Holds for 1 exchange only
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 11
Rosenbluth separationRosenbluth separation
=05=02
=08
Contribution of the electric term
hellipto be compared to the absolute value of the error on and to the size and dependence of RC
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 12
The polarization induces a term in the cross section proportional to GE GM
Polarized beam and target or
polarized beam and recoil proton polarization
The polarization method (1967)The polarization method (1967)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 13
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 14
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 11
Rosenbluth separationRosenbluth separation
=05=02
=08
Contribution of the electric term
hellipto be compared to the absolute value of the error on and to the size and dependence of RC
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 12
The polarization induces a term in the cross section proportional to GE GM
Polarized beam and target or
polarized beam and recoil proton polarization
The polarization method (1967)The polarization method (1967)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 13
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 14
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 12
The polarization induces a term in the cross section proportional to GE GM
Polarized beam and target or
polarized beam and recoil proton polarization
The polarization method (1967)The polarization method (1967)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 13
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 14
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 13
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 14
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 14
Neutron Form Factors
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 15
The reaction d(eersquon)p - Ax
Select quasi-elastic kinematics
Pol electron beam pol target orneutron polarimeter
Large dependence ofasymmetry on GEn
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
+ d n + p
DWF
GEn
GEp
FSI
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 16
The reaction d(eersquon)p - Ax
-The KHARKOV model - Impulse Approximation - Deuteron structure - Kinematics proton spectator - Polarization observables
GI Gakh A P Rekalo E T-G Annals of Physics 319 150 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 17
FSI
DWF
Does not depend on beam helicity
+ d n + pGEn
ET-G GI Gakh A P Rekalo M P Rekalo PRC70025202 (2004)
The reaction d(eersquon)p ndash AxAz
Generalization of the polarization method
Asymmetry ratio
A(01)T ndashLT SFs(WQ2)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 18
GEn from the deuteron
bullGEn gt GEp starting from 2 GeV2
E T-G and M P Rekalo Europhys Lett 55 188 (2001)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 19
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 20
STATUS on EM Form factors
Space-like region
1) standard dipole function for the nucleon magnetic FFs GMp and GMn
2) linear deviation from the dipole function for the electric proton FF GEp
3) contradiction between polarized and unpolarized measurements
4) non vanishing electric neutron FF GEn
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 21
Nucleon models
bullSkyrme Models (Soliton)bullVector Dominance Models (G-K IJLhellip)bullPerturbative QCDbull(Relativistic) Constituent Quark ModelbullDi-quark modelsbullGPDbullhelliphellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 22
The nucleon form factors
VDM IJLF IachelloPLB 43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC 66 045501 2002)
HohlerNPB 114 505 (1976)
BostedPRC 51 409 (1995)
Electric Magneticne
utro
npr
oton
E T-G F Lacroix Ch Duterte GI Gakh EPJA 24 419 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 23
Time-like region
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 24
Time-like observables | GE| 2 and | GM| 2
As in SL region- Dependence on q2 contained in FFs- Even dependence on cos2exchange- No dependence on sign of FFs- Enhancement of magnetic term
but TL form factors are complex
A Zichichi S M Berman N Cabibbo R Gatto Il Nuovo Cimento XXIV 170 (1962)B Bilenkii C Giunti V Wataghin Z Phys C 59 475 (1993)G Gakh ET-G Nucl Phys A761120 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 25
Time-Like Region
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419 (2005)
VDM IJLF IachelloPLB43 191 (1973)
Extended VDM (G-K 92) ELLomon PRC66 045501(2002)
lsquoQCD inspiredrsquo
proton
neutron
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 26
STATUS on EM Form factors
Time-like region
1) No individual determination of GE and GM2) Assume GE=GM (valid only at threshold) VMD or
pQCD inspired parametrizations (for p and n)
3) TL nucleon FFs are twice larger than SL FFs 4) Recent data from Babar (radiative return)
bull interesting structures in the Q2 dependence of GM(=GE)
bull GMneGE
=03 GeV is the QCD scale parameter
A(p) = 563 GeV4 A(n) = 7715 GeV4
)](ln[ 2222
ss
AGM
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 27
Spin Observables
Analyzing power A
Double spin observables
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 28
Models in TL Region (polarization)
VDM IJL
Ext VDM
lsquoQCD inspiredrsquo
R
Ay Axx Ayy
Axz
Azz
E T-G F Lacroix C Duterte GI Gakh EPJA 24 419(2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 29
Time-Like Region GE versus GM
GE=0
GE=GM
GE=GD
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Asym
| GM| 2
Cross section at 900
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 30
Perspectives in Time-Like region
Frascati
Panda
GE = GM
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
CEA DSM Dapnia
Facilty for Antiproton and Ion Research (GSI Darmstadt Germany)
- Proton linac (injector)- 2 synchrotons (30 GeV p)- A number of storage rings Parallel beams operation
Physics Polarization Staging Signals Timeline
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 32
Towards a unified description of Hadron Form factors
to clarify
- zero of GEp
- asymptotic properties
- reaction mechanism
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 33
Comparison BABAR-LEAR
q2 (GeV2)
Analytical Expression for R(q2)Dispersion Relations (S Pacetti)
Space-like Time-like
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 34
Phragmegraven-Lindeloumlf theorem
Asymptotic properties for analytical functions
E T-G and G Gakh Eur Phys J A 26 265 (2005)
=005 01
If f(z) a as z along a straight line and f(z) b as z along another straight line and f(z) is regular and bounded in the angle between then a=b and f(z) a uniformly in the angle
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 35
Phragmegraven-Lindeloumlf theorem
E T-G and M P Rekalo Phys Lett B 504 291 (2001)
Applies to NN and NNInteraction (Pomeranchuk theorem )t=0 not a QCD regime
Connection with QCD asymptoticsGM (TL)
GM (SL)
GE (SL)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 36
Reaction mechanism1-2 interference
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 37
Two-photon exchange
Different results with different experimental methods
- Both methods based on the same formalism
- Experiments repeated
New mechanism
bull1-2 ~ =e24=1137
bull1970rsquos Gunion Levhellip
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 38
eeplusmn plusmn + p+ prarr rarr eeplusmnplusmn + p+ p
1 exchange
bull Two EM form factorsbull Real (in SL region)bull Functions of one variable (t)bull Describe e+ and e- scattering
2 exchange
bull Three structure functionsbull Complexebull Functions of TWO variables (st)bull Different for e+ and e- scattering
4 spin frac12 fermions rarrrarr 16 amplitudes in the general caseT-invariance of EM interaction identity of initial and final states helicity conservation unitarity
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 39
Model independent considerations for eeplusmnplusmn N scattering
Determination of EM form factors in presence of 2 exchange
-electron and positron beams
- longitudinally polarized - in identical kinematical
conditions
M P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 40
Model independent considerations for eeplusmnplusmn N scattering
If no positron beamhellip
Either three T-odd polarization observableshellip
bullAy unpolarized leptons transversally polarized target (or Py outgoing nucleon polarization with unpolarized leptons unpolarized target )bullDepolarization tensor (Dab) dependence of the b-component of the final nucleon polarization on the a-component of the nucleon target with longitudinally polarized leptonsor five T-even polarization observableshellip
among dsd Pxe) Pz(e) Dxx Dyy Dzz DxzM P Rekalo E T-G EPJA (2004) Nucl Phys A (2003)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 41
1g
1-2 interference
21
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 42
The 1-2 interference destroys the linearity
of the Rosenbluth plot
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 43
11-2-2 interference (e-d) interference (e-d)
M P Rekalo E T-G and D Prout Phys Rev C60 042202 (1999)
CA DA
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 44
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 45
From the data
deviation from linearity
ltlt 1
Parametrization of 2-contribution for e+p
E T-G G Gakh Phys Rev C 72 015209 (2005)
)(1
1)( 2)(2 QfQF a
2222
22
]1[ a
Dγ(a)
m[GeV]Q
GC)(Qf
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 46
Two-Photon exchange
bullThe 2 amplitude is expected to be mostly imaginary
bullIn this case the 1-2 interference is more important in time-like region as the Born amplitude is complex
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 47
TL unpolarized cross section
bullInduces four new termsbullOdd function of bullDoes not contribute at =90deg
2contribution
e+ +e- p + p
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 48
bullProperties of the TPE amplitudes with respect to the transformation cos = - cos ie -
(equivalent to non-linearity in Rosenbluth fit)
bullBased on these properties one can remove or single out TPE contribution
Symmetry relationsSymmetry relations
E T-G G Gakh NPA (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 49
bullDifferential cross section at complementary angles
Symmetry relations
The DIFFERENCE enhances the 2 contribution
The SUM cancels the 2 contribution
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 50
Radiative Return (ISR)
s
m
x
sin
xx
x)xs(W
s
m
s
Ex)m)(ppee()xs(W
s
m
cosddm
)ppee(d
e
2
22
122
2
2
2
2
e+ +e- p + p +
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 51
Angular distribution
Mpp=1877-19Mpp=1877-19
Mpp=24-3Mpp=24-3
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 52
Mpp=1877-19Mpp=1877-19
A=001A=001plusmnplusmn002002
Mpp=24-3Mpp=24-3
E T-G EA Kuraev S Bakmaev S Pacetti Phys Lett B (2008)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 53
Radiative Corrections to the dataRadiative Corrections to the data
Slope negative if
- RC can reach 40 on - Declared error ~1- Same correction for GE and GM
- Have a large -dependence- Affect the slope
The slope is negative starting from 2-3 GeV2
el=meas RC
slope
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 54
Reduced cross section and RCReduced cross section and RCData from L Andivahis et al Phys Rev D50 5491 (1994)
Q2=175 GeV2
Q2=5 GeV2
Q2=325 GeV2
Q2=4 GeV2
Q2=25 GeV2
Q2=7 GeV2
Q2=6 GeV2
Radiative Corrected data
Raw data without RC
Slope from P M
E T-G G Gakh PRC 72 015209 (2005)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 55
Scattered electron energy
All orders of PT needed beyond Mo amp Tsai approximation
Initial state emission
final state emission
Quasi-elastic scattering
3
Y0
Not so smallShift to LOWER Q2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 56
Radiative Corrections (SF method)
Polarization data
JLab data
SLAC data
Yu Bystricky EAKuraev E T-G Phys Rev C75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 57
Instead of Conclusionshellip
bullFundamental measurement the electric and the magnetic distributions of the proton are different in SL region What about TL Separation of GE and GM
via angular dependence of differential cross section
bull Clarify reaction mechanism 2- exchange by model independent symmetry requirements
bull Unified description in TL and SL region zero of GEp
bull Asymptotic properties QCD and analyticity
Model independent propertiesModel independent properties Lessons from QED Lessons from QED
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 58
The work presentedhere was initiated in a collaboration with Prof M P REKALO
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 59
Experimental correlationExperimental correlation
el=meas RC
Q2 gt 2 GeV2 Q2 lt 2 GeV2
RC()
only published values
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 60
Experimental correlationExperimental correlation
Q2 lt 2 GeV2
Correlation (ltRCbull)
ET-G Phys Part Nucl Lett 4 281 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 61
The Pauli and Dirac Form Factors
Normalization
F1p(0)=1 F2p(0)= κp
GEp(0)=1 GMp(0)=μp=279
The electromagnetic current in terms of the Pauli and Dirac FFs
Related to the Sachs FFs
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 62
Two Photon Exchange
No exact calculation for ep scattering
( inelastic intermediate states)
but
electron-muon scattering
constitutes an upper limit
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 63
Interference of 1 2 exchange
bullExplicit calculation for structureless proton ndash The contribution is small for unpolarized and
polarized ep scatteringndash Does not contain the enhancement factor L ndash The relevant contribution to K is ~ 1
EAKuraev V Bytev Yu Bystricky ET-G Phys Rev D74 013003 (1076)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 64
QED versus QCD
Imaginary part of the 2Imaginary part of the 2 amplitude amplitude
electronproton
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 65
QED versus QCD
Q2=005 GeV2
Q2=12 GeV2
Q2=2 GeV2
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 66
Structure Function method
bullSF method applied to QED processes calculation of radiative corrections with precision of 01
bullTakes into account the dynamics of the process
bullFormulated in terms of parton densities (leptons antileptons photons)
bullMany applications to different processes
E A Kuraev and VS Fadin Sov J of Nucl Phys 41 466 (1985)
Electron SF probability to lsquofindrsquo electron in the initial electron with energy fraction x and virtuality up to Q2
Lipatov equations (1975)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 67
Unpolarized Cross sectionUnpolarized Cross section
Born +dipole FFs(=unpolarized experiment+MoampTsai)
SF (with dipole FFs)SF+2 exchange
Q2=3 GeV2
Q2=5 GeV2 SF change the slope
Q2=1 GeV2
2 exchange very small
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)
Egle TOMASI-GUSTAFSSONCEA DSM DapniaJLab May 22008 68
Polarization ratioPolarization ratio
Born SFSF+2 exchange
=60deg
2 destroys linearity
2 exchange very small
=80deg
=20deg
Yu Bystricky EAKuraev E T-G Phys Rev C 75 015207 (2007)