quark gluon interactions and partonic angular momentum€¦ · quark gluon interactions and...
TRANSCRIPT
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Quark Gluon Interactions and Partonic Angular Momentum
September 16, 2019
POETIC 2019Lawrence Berkeley National Laboratory
Abha RajanBrookhaven National Laboratory
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Collaborators
● Simonetta Liuti (University of Virginia)
● Michael Engelhardt (New Mexico State University)
● Aurore Courtoy (Mexico University)
● Tyler Gorda (University of Virginia)
● Kent Yagi (University of Virginia)
Orbital Angular Momentum
Equation of State Neutron stars
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Outline
● Partonic Orbital Angular Momentum
● Wandzura Wilczek and genuine twist three contributions to twist three GPDs
● Role of gauge link
● Extending to chiral odd sector
● Results on the equation of state of neutron stars at short distances
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Proton Spin Crisis
Spin Crisis !!!
Quark Spin Contribution
What are other sources ?Partonic Orbital Angular Momentum
Measured by EMC experiment in 1980s to be small, present values about 30% of total !!
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QCD Energy Momentum Tensor
QCD Lagrangian
Energy Momentum Tensor
Momentum Angular Momentum Energy density, Pressure
Observables
Deeply Virtual Compton Scattering, moments of GPDs etc.
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QCD Energy Momentum Tensor
Energy Momentum
Pressure Shear stress
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QCD Energy Momentum Tensor
Energy Momentum
Pressure Shear stress
Angular Momentum
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QCD Energy Momentum Tensor
Energy Momentum
Pressure Shear stress
Angular Momentum
Xiangdong Ji, PRL 78.610,1997
Partonx
bT
Angular Momentum described by GPDs which are collinear
OAMSpinTotal
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Do we have a direct description of orbital angular momentum ?
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Partonic Orbital Angular Momentum
Kiptily and Polyakov, Eur Phys J C 37 (2004)
● The moment in x of the GPD G2 shown to be OAM● Twist three GPD, implicitly includes quark gluon interactions
Hatta and Yoshida, JHEP (1210), 2012
Twist 3
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● Consider measuring both the intrinsic transverse momentum and the spatial distribution of partons
● Lq,z = bT X kT
x, kT
bT
Lz
Generalized Transverse Momentum Distributions (related by Fourier transform to Wigner Distributions) Meissner Metz and Schlegel,
JHEP 0908 (2009)
Partonic Orbital Angular Momentum II
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The Two Definitions
● Weighted average of bT X kT
● Difference of total angular momentum and spin
GTMD
GPD
Lorce, Pasquini (2011)
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Distribution of OAM in x
● We find that
● This is a form of Lorentz Invariant Relation (LIR)● This is a distribution of OAM in x● Derived for a straight gauge link
AR, Engelhardt and Liuti PRD 98 (2018) AR, Courtoy, Engelhardt and Liuti PRD 94 (2016)
Twist two Twist three
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Derivation of Generalized LIRs
Integrate over
Integrate over
GTMDs
GPDs
Generalized Parton Correlation Functions (GPCFS)
Meissner Metz and Schlegel, JHEP 0908 (2009)
To derive these we look at the parameterization of the quark quark correlator function at different levels
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Generalized Lorentz Invariance Relations
● Parametrization of the quark quark correlator at different levels
● LIRs occur because the number of GPCFs is less than the number of GTMDs.
Explicit kT coefficientIntegrate over
Integrate over
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Generalized Lorentz Invariance Relations
The GTMDs are complex in general.
The imaginary part integrates to zero, on integration over kT.
Axial Vector
Vector
Twist two Twist three
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Generalized Lorentz Invariance Relations
● As the quark quark correlator is non-local, the parameterization depends on the choice of gauge link.
● At the completely unintegrated level, we have no knowledge of the light-cone direction if we consider a straight gauge link.
● This is at variance with the staple gauge link case – even at the completely unintegrated level introduction of the N- vector along which the staple lies introduces more functions that parameterize the correlator.
● As a result we need to introduce the LIR violating term. Gauge Link
Completely unintegrated correlator
straight staple
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Generalized Lorentz Invariance Relations
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LIR violating term
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LIR violating term
staple straight
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Intrinsic Momentum vs Momentum Transfer
Courtoy et al PhysLett B731, 2013
Burkardt,Phys Rev D62, 2000
P P'
k k'
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Intrinsic Momentum vs Momentum Transfer
Courtoy et al PhysLett B731, 2013
Burkardt,Phys Rev D62, 2000
P P'
k k'
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Equations of Motion Relations
How do we obtain these ?
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Equations of Motion Relations
How do we obtain these ?
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Equations of Motion Relations
How do we obtain these ?
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Equations of Motion Relations
How do we obtain these ?
Crucial for understanding qgq contribution to GPDs!!
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Use LIRs and Equation of Motion Relations to derive Wandzura
Wilczek Relations● The equations of motion connect kT dependent
quantities with collinear objects.
● These kT dependent quantities are also connected to collinear objects by LIRs. This is independent of equation of motion relations.
● Use the LIR to eliminate the kT dependent quantities in equation of motion relations. This results in the Wandzura Wilczek relations for twist 3 GPDs.
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EoM relations for Orbital Angular Momentum
Twist 3 Twist 2 Genuine Twist 3 (explicit gluon)
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Wandzura Wilczek Relations
Twist three vector GPD
Twist twoAxial vector GPD contributes to a vector GPD
Genuine Tw 3
Twist three PDF Twist two
Genuine Tw 3
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Role of Gauge Link Equation of Motion
GPDs are not affected by staple Eliminated using LIRQuark gluon quark correlator - affected by choice of gauge link
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Role of Gauge Link Equation of Motion
GPDs are not affected by staple Eliminated using LIRQuark gluon quark correlator - affected by choice of gauge link
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Role of Gauge Link – calculations in the diquark model
With Brandon Kriesten and Simonetta Liuti
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Back to Wandzura Wilczek Relations
staple
straight
GPDs are collinear. They carry no memory of the staple gauge link.
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Equation of state of Neutron Stars at Short Distances
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QCD Energy Momentum Tensor
Energy Momentum
Pressure Shear stress
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Energy Momentum Tensor Parameterization
● The quark and gluon contributions to the energy momentum tensor are parameterized by the gravitational form factors.
Off forward Quark and gluon contributions not conserved separately
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GPD moments and the EMT
● Mellin moments of GPDs give the gravitational form factors that parameterize the energy momentum tensor.
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GPD moments and the EMT
● Mellin moments of GPDs give the gravitational form factors that parameterize the energy momentum tensor.
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GPD moments and the EMTMoments
Physical Interpretation
Angular Momentum
Internal Forces
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D-term and pressure
shear pressure
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Pressure Distribution inside the Proton
Detmold and Shanahan (PRL, 2019)Burkert, Elouadrhiri, Girod (Nature, 2018)
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Neutron Stars
Gravitational collapse is countered by pressure generated by nuclear forces
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Equation of State of Neutron Stars
S Liuti, AR, K Yagi, T Gorda arxiv:1812.01479
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Conclusions
● Way of deriving the Wandzura Wilczek relations. Allows us to write out precisely quark gluon contribution to twist 3. Study x dependence.
● Gluons play a key role in the mass and pressure make up of the proton – even neutron stars!
● Quark gluon quark interactions are at the heart of unravelling the structure of the proton.
Thank you!
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OAM
Genuine Twist Three
Moments of twist three GPDs -Quark gluon structure
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Moments of twist three GPDs -Quark gluon structure
mass term
Genuine Twist Three
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Quark gluon quark contributions
straight staple
(final state interactions)
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Calculating the force from Lattice data – Sivers function
The derivative with respect to the gauge link direction gives the force!
Transversely polarized proton
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Michael Engelhardt
Phys. Rev. D95 (2017)
Straight link
Staple
Torque!
Longitudinally polarized proton
Calculating the torque from Lattice
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Experimental measurements
The production of a heavy quarkonium near threshold in electron-proton scattering is connected to the origin of the proton mass via the QCD trace anomaly.
Calculate cross-section using input from latest lattice QCD calculations of gluon gravitational form factors.
D.E Kharzeev (1995)
Y Hatta, DL Yang PRD98 (2018)
Detmold and Shanahan arxiv:1810:04626In an actual experiment
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Equation of state of Neutron Stars at Short Distances
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Pressure Distribution inside the Proton
Detmold and Shanahan (PRL, 2019)Burkert, Elouadrhiri, Girod (Nature, 2018)
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Equation of State of Neutron Stars
S Liuti, AR, K Yagi arxiv:1812.01479
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Conclusions
● Way of deriving the Wandzura Wilczek relations. Allows us to write out precisely quark gluon contribution to twist 3. Study x dependence.
● Gluons play a key role in the mass and pressure make up of the proton – even neutron stars!
● Quark gluon quark interactions are at the heart of unravelling the structure of the proton.
Thank you!
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Thanks!
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Higher Twist
Leading twist – twist 2
● Involve only good components
● Simple interpretation in terms of parton densities
Higher twist – twist 3
● Involve one good and one bad component
● The bad component represents a quark gluon composite
P P'
k k'
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Collinear Picture : Transverse Quark Current, Higher Twist
Leading order quark current
Transverse quark current, implicitly involves quark gluon interactions
Probabilistic parton model interpretation works well at leading order, with transverse quark projection operator need to include quark gluon interactions
Both in Collinear Picture
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Quark and gluon contributions to the trace anomaly
Trace
renormalization
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Equations of Motion Relations
How do we obtain these ?
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Derivation of Generalized LIRs
Integrate over
Integrate over
GTMDs
GPDs
Generalized Parton Correlation Functions (GPCFS)
Meissner Metz and Schlegel, JHEP 0908 (2009)
To derive these we look at the parameterization of the quark quark correlator function at different levels
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Generalized Lorentz Invariance Relations
Distribution of OAM in x !
moment of a twist two function
Twist three function
● The same set of As describe the whole vector sector.
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Generalized Lorentz Invariance Relations
Axial Vector
Vector
Twist two Twist three
Intrinsic transverse momentum
Quark gluon interactions
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EoM relations for Orbital Angular Momentum
Twist 3 Twist 2 Genuine Twist 3 (explicit gluon)
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Moments of twist three GPDs -Quark gluon structure
mass term
Genuine Twist Three
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Staple gauge link
straight staple
(final state interactions)
Gauge link
Non local operator
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LIR violating term
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Understanding the mass decomposition of the proton
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Mass decomposition of the proton
Traceless
Rest frame
X Ji (1995)
Traceless
Trace part
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Energy Momentum Tensor Parameterization
● The full energy momentum tensor is a conserved quantity and is scale independent.
● The separate contributions from the quarks and gluons on the other hand are not and do depend on the renormalization scale.
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Trace Anamoly Total
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Trace Anamoly
Trace
Total
Quark and gluon components separated
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Trace Anamoly
Trace
Trace
By studying the Gravitational form factors A and C we will know the quark and gluon contributions to the trace anomaly separately.
Total
Quark and gluon components separated
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Quark and gluon contributions to the trace anomaly
Trace
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Quark and gluon contributions to the trace anomaly
Trace
gluons quarks
Y Hatta, AR, K Tanaka, JHEP 1812 (2018) 008