scattering and annihilation processespacetti/trento13/talks/egle-trento13.pdf · scattering and...
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Egle Tomasi-Gustafsson
Simone Pacetti
Marco Maggiora
Trento, ECT*, February 18-22, 2013
Scattering and Annihilation Processes
ECT* 21/II/2013 1 Egle Tomasi-Gustafsson
Time-like and Space-like Hadron Form Factors
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Egle Tomasi-Gustafsson ECT* 21/II/2013 2
Three general introductory talks Diego Bettoni, Frank Maas, Rinaldo Baldini
Purpose of the workshop
Gather experimentalists and theoreticians from different communities: electron, hadron accelerators and colliders
Progress on the way of having a unified and coherent description of hadron electromagnetic FFs in the whole kinematical region
Triggered by recent precise data : ep-scattering (Jlab), e+e- ( Novosibirsk, BESIII) and future pbar+p (PANDA, FAIR)
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ECT* 21/II/2013 Egle Tomasi-Gustafsson 3
Le Monde, July 2012: the Word of the Month: HIGGS BOSON
F. Maas
Static: Origin of nucleon mass Quark and gluon condensate Dynamics: Structure of the nucleon: form factors
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Hadron Form Factors: a long history
The ’Kharkov’ school The ’Italian’ school The ‘Russian’ school
SLAC, JLAB
Characterize the internal structure of a particle ( point-like)
Elastic form factors contain information on the hadron ground state.
In a P- and T-invariant theory, the EM structure of a particle of spin S is defined by 2S+1 form factors.Playground for theory and experiment
at low q2 probe the size of the nucleus, at high q2 test QCD scaling
Experiments and Theory: France,Germany
…some names are UNAVOIDABLE in references!
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The proton vertex is parametrized in terms of FFs: Pauli and Dirac F1,F2
Electromagnetic Interaction
q2<0
e- e-
p p )2q(
2F
M2
qi)2q(
1F
or in terms of Sachs FFs: GE=F1+t F2, GM=F1+F2, t=q2/4M2
The electron vertex is known,
The interaction is carried by a virtual photon of mass2 q2
What about high order radiative corrections? Egle Tomasi-Gustafsson
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Egle Tomasi-Gustafsson ECT* 21/II/2013 7
Crossing Symmetry
Scattering and annihilation channels:
- Described by the same amplitude :
- function of two kinematical variables, s and t
k2 → – k2
- which scan different kinematical regions
p2 → – p2
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Egle Tomasi-Gustafsson ECT* 21/II/2013 8
Analyticity
_ _
q2<0
e- e-
p p
q2>0
e-
e+ p
p
q2 q2=4mp2
FFs are complex FFs are real
Un
ph
ysic
al r
egio
n
GE=GM
Space-like
Time-like GE(0)=1
GM(0)=p
Asymptotics - QCD - analyticity
p+p ↔ e++e- e+p e+p
p+p
↔ e
++e
- +p
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Egle Tomasi-Gustafsson 9
The Rosenbluth separation
)2(2)2(2
)1(
1Q
MGQ
EG
Mott
d
d
d
d
t
t
2M4
2Q
,
1
2
e2)tan1(21
t
t
2M
G2E
GR
t
Holds for 1 exchange only
Linearity of the reduced cross section
PRL 94, 142301 (2005)
tan2e dependence
Q2 f
ixed
ECT* 21/II/2013
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Egle Tomasi-Gustafsson 10
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)
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The simultaneous measurement of Pt and Pl reduces the systematic errors
The polarization method (exp)
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C. Perdrisat et al, JLab-GEp collaboration
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Polarization experiments - Jlab A.I. Akhiezer and M.P. Rekalo, 1967
GEp collaboration 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) QCD scaling not reached
3) Zero crossing of Gep?
4) contradiction between polarized and unpolarized measurements
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A.J.R. Puckett et al, PRL (2010)
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Gep III results (2010)
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QED Radiative Corrections
Egle Tomasi-Gustafsson ECT* 21/II/2013 14
Modify the absolute value of the experimental observables and their dependence from the relevant kinematical variables
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Egle Tomasi-Gustafsson ECT* 21/II/2013 15
Radiative Corrections (ep)
RC to the cross section: large (may reach 40%) and Q2 dependent calculated at first order
May change the slope of R
(and even the sign !!!)
Q2=5 GeV2
Q2=3.75 GeV2
Q2=1.75 GeV2
E. T.-G., G. Gakh, PRC72, 015209 (2005), C.F Perdrisat et al, Progr.Part.Nucl.Phys.(2010)
Andivahis et al., PRD50, 5491 (1994)
2M
G2E
GR
t
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First order Radiative Corrections (ep)
Mo&Tsai (1969) - Maximon&Tjon (2000)
E.A. Kuraev et al,
The difference - is epsilon-dependent - increases with Q2
Q2=5 GEV2
V. Fadin
e-Print: arXiv:0805.3623 [hep-ph] |
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Egle Tomasi-Gustafsson ECT* 21/II/2013 18
Why higher orders?
All orders of PT needed
beyond Mo & Tsai approximation!
Initial state emission
final state emission
Quasi-elastic scattering
3%
Y0
Not so small!
Shift to LOWER Q2
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Egle Tomasi-Gustafsson ECT* 21/II/2013 19
The Structure Function Method
Distinguish: -leading contributions of higher order
-non leading ones
E. A. K. and V.S. FADIN, Sov. J. of Nucl. Phys. 41, 466 (1985)
The SF method is based on: • Renormalization group evolution equation
• Drell-Yan parton picture of the cross section in QCD
Electron SF: probability to ‘find’ electron in the
initial electron, with energy fraction x and virtuality up to Q2
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Egle Tomasi-Gustafsson ECT* 21/II/2013 20
The LSF cross section (for ep ) •If the electron is detected in a calorimeter: the cross
section is integrated over the scattered electron energy
fraction:
•The K-factor includes all non leading contributions (2,…):
1),z(Ddz
1
0
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Egle Tomasi-Gustafsson ECT* 21/II/2013 21
LSF: ‰ precision
2
e
2
m
QlnL,1L
p
%2.0
400
1L
p
p
E. A. K. and V.S. FADIN, Sov. J. of Nucl. Phys. 41, 466 (1985)
LLA (Leading Logarithm Approximation)
Precision of LLA
%01.0L
2
p
p
Even when corrections in first order PT are d~100%, the accuracy of higher order RC (LSF) is /p d1% !
Including K-factor
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A common effort for RC and Monte Carlo tools ~60 participants, 13 countries www.lnf.infn.it/wg/sighad
(next meeting 11-12 April 2013, ECT*) – G. Venanzoni
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Egle Tomasi-Gustafsson 23
e± + p→ e± + p
1 exchange
• Two EM form factors • Real (in SL region) • Functions of one variable (t) • Describe e+ and e- scattering
2 exchange
• Three structure functions • Complexe • Functions of TWO variables (s,t) • Different for e+ and e- scattering
4 spin ½ fermions → 16 amplitudes in the general case. T-invariance of EM interaction, identity of initial and final states, helicity conservation, unitarity
1. Interference 1- 2
2. ‘Hard’ 2 box 3. 6% effect needed
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Gep III results (2010)
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Bystritskiy SF
No radiative corrections applied to the data
No evidence of large two photon effects
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Egle Tomasi-Gustafsson 30
Issues • Some models (IJL 73, Di-quark,
soliton..) predicted such behavior before the data appeared
• Simultaneous description of the four nucleon form factors...
• ...in the space-like and in the time-like regions
• Consequences for the light ions description
• When pQCD starts to apply?
• Source of the discrepancy
BUT
ECT* 21/II/2013
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Egle Tomasi-Gustafsson ECT* 21/II/2013 33
Point-like form factors?
S. Pacetti R. Baldini
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2) The vacuum state transfers all the released energy to a state of matter consisting of:
• 6 massless valence quarks • Set of gluons • Sea of current qq pairs of quarks with energy q0>2Mp, J=1, dimensions
Annihilation channel:
Egle Tomasi-Gustafsson ECT* 21/II/2013 36
3) Pair of p and p formed by three bare quarks: •Structureless •Colorless pointlike FFs !!!
1) Creation of a pp state through intermediate state with
E. A. Kuraev
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The annihilation channel:
Egle Tomasi-Gustafsson ECT* 21/II/2013 37
• The point-like hadron pair expands and cools down: the current quarks and antiquarks absorb gluon and transform into constituent quarks
• The residual energy turns into kinetic energy of the motion with relative velocity
• The strong chromo-EM field leads to an effective loss of color. Fermi statistics: identical quarks are
repulsed. The remaining quark of different flavor is attracted to one of the identical quarks, creating a compact diquark (du-state)
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The annihilation channel:
Egle Tomasi-Gustafsson ECT* 21/II/2013 38
The neutral plasma acts on the distribution of the electric charge (not magnetic).
Prediction: additional suppression due to the neutral plasma similar behavior in SL and TL regions
• Implicit normalization at q2=4Mp2: |GE|=|GM| =1
• No poles in unphysical region
E.A. Kuraev et al., Phys.Lett. B712 (2012) 240-244
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Egle Tomasi-Gustafsson ECT* 21/II/2013 39
Proton Form Factors
GMp
GEp Akhiezer-Rekalo
GEp Rosenbluth |GMp|=|GEp|
E.A. Kuraev et al., Phys.Lett. B712 (2012) 240-244
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E. Santopinto
Relativistic constituent quark models
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A. Drago
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A. Drago
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G. Salmè
Extension to time-like!
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ECT* 21/II/2013 Egle Tomasi-Gustafsson 45
G. Salmè Time-like
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ECT* 21/II/2013 Egle Tomasi-Gustafsson 46
G. Salmè
Space-like
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ECT* 21/II/2013 Egle Tomasi-Gustafsson 47
M. Radici
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ECT* 21/II/2013 Egle Tomasi-Gustafsson 48 M. Radici
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TMD: KT-dependent Parton Distributions
Twist-2 PDFs )k,x(fkd)x(fT1T
2
1
Distribution
functions Chirality
even odd
Twist-2
U
L
T
,
h1,
Transversity
Boer-Mulders
Sivers
1h
L1h
T1h
Tf
1 Tg
1
1f
1g
ECT* 21/II/2013 49 Egle Tomasi-Gustafsson M. Destefanis
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Drell-Yan Process
• Drell-Yan: pp -> +-X
Collins-Soper frame
Kinematics
x1,2 = mom fraction of parton1,2
t = x1 • x2 = M2/s
xF = x1 - x2
Collins-Soper frame: Phys. Rev. D16 (1977) 2219. ECT* 21/II/2013 50 Egle Tomasi-Gustafsson
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SINGLE-POLARISED
UNPOLARISED
.
DOUBLE-POLARISED
Drell-Yan Cross Section
R.D. Tangerman and P.J. Mulders, Phys. Rev. D51, 3357-3372 (1995) ECT* 21/II/2013 51 Egle Tomasi-Gustafsson
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Azimuthal Asymmetries
)2cos(
)sin(),sin(
2cos
21
22
SS
SS
• Unpolarized
• Single polarized
• Double polarized
U = N(cos2φ>0)
D = N(cos2φ<0) DU
DUA
Asymmetry
ECT* 21/II/2013 52 Egle Tomasi-Gustafsson
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DY Asymmetries @ Vertex
UNPOLARISED SINGLE-POLARISED
500KEv included in asymmetries
Acceptance corrections
crucial!
1 < qT < 2 GeV/c
2 < qT < 3 GeV/c
xP xP
xP
xP
xP xP
Physics Performance Report for PANDA arXiv:0903.3905 ECT* 21/II/2013 53 Egle Tomasi-Gustafsson
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R = L ·σ·ɛ
= 2·1032cm-2s-1 ×
x 0.8·10-33cm2× 0.33
= 0.05 s-1 ~ 130 Kev/month
Statistical errors for 500KEv generated
xP
)
)
xP
xP Physics Performance Report for PANDA arXiv:0903.3905
DY Asymmetries @ Vertex
ECT* 21/II/2013 54 Egle Tomasi-Gustafsson
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ECT* 21/II/2013 Egle Tomasi-Gustafsson 55 A. Dbeyssi
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ECT* 21/II/2013 Egle Tomasi-Gustafsson 56
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ECT* 21/II/2013 Egle Tomasi-Gustafsson 57
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Egle Tomasi-Gustafsson ECT* 21/II/2013 58
Radiative Return (ISR)
.
s
m,
x
sin
xx
x
),x,s(W
,
s
m
s
E
x),m)(ppee(),x,s(W
s
m
cosddm
)ppee(d
e
p
2
22
1
22
2
2
2
2
e+ +e- p + p +
B. Aubert ( BABAR Collaboration) Phys Rev. D73, 012005 (2006)
Application to BES-III presented by:
F. Maas on behalf of C. Morales
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ECT* 21/II/2013 59
Time-like observables: | GE| 2 and | GM| 2 .
As in SL region: - Dependence on q2 contained in FFs - Even dependence on cos2 (1 exchange) - 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, E.T-G., Nucl. Phys. A761,120 (2005).
Egle Tomasi-Gustafsson
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ECT* 21/II/2013
Individual determination of GE and GM up to large Q2
Expected Results
R=GE/GM
BaBAR
PS170 PANDA sim
M. Sudol et al, EPJA 2010
Egle Tomasi-Gustafsson 60
L = 2 10 32 cm2 s1
100 days
new PandaRoot analysis Mainz, Orsay D. Khaneft
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ECT* 21/II/2013 Egle Tomasi-Gustafsson 61 Added material following the discussion
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ECT* 21/II/2013 Egle Tomasi-Gustafsson 62 Added material following the discussion
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ECT* 21/II/2013 Egle Tomasi-Gustafsson 63
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Egle Tomasi-Gustafsson ECT* 21/II/2013 64
Hadron Form Factors: Conclusions
Large activity in Space-like and Time-like regions
IHEP
VEPP-3 Novosibirsk
To measure:
• zero crossing of GE/GM in SL? 2? Proton radius • GE and GM separately in TL • complex FFs in TL region: polarization!
Unified models in SL and TL regions: • reproduce proton, neutron, electric, magnetic • pointlike behavior at threshold? •GEn, GMn(SL)<GEn,GMn(TL);
Jefferson Lab
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ECT* 21/II/2013 Egle Tomasi-Gustafsson 65
Thank you for attention