CHAPTER 13 Kinetics of Particles: Energy and Momentum Methods Energy and Momentum Methods.
Quark spin-orbit correlations - Jefferson Lab...Energy-momentum tensor A lot of interesting physics...
Transcript of Quark spin-orbit correlations - Jefferson Lab...Energy-momentum tensor A lot of interesting physics...
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Cédric Lorcé
IPN Orsay - IFPA Liège
Quark spin-orbit correlations
May 14th 2014, Santa Fe, New Mexico, USA
[C.L., arXiv:1401.7784]
[C.L., Pasquini (in preparation)]
Based on :
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Outline
• Energy-momentum tensor
• Quark spin-orbit correlations
• Phase-space transverse modes
• Conclusions
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Energy-momentum tensor
A lot of interesting physics is contained in the EM tensor
Energy density
Momentum density
Energy flux
Momentum flux
Shear stress
Normal stress (pressure)
E.g.
[Polyakov, Shuvaev (2002)]
[Polyakov (2003)]
[Goeke et al. (2007)]
[Cebulla et al. (2007)]
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Energy-momentum tensor
Momentum-space expression
General parametrization
Non-conservation
Asymmetry
[Ji (1997)]
[Shore, White (2000)]
Angular momentum
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Link with GPDs
« Trick »
Local Non-local
GPD operator
[Penttinen et al. (2000)]
[Kiptily, Polyakov (2004)]
[Hatta, Yoshida (2012)]
Twist-2
Twist-3
[Ji (1997)]
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Proton spin structure
« Quark spin »
« Quark OAM »
Quark spin-orbit correlation
[C.L., Pasquini (2011)] [C.L. (2014)]
Not involved in proton spin sum rule !
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Proton spin structure
« Quark spin »
« Quark OAM »
Quark spin-orbit correlation
[C.L., Pasquini (2011)] [C.L. (2014)]
Quark number
UU
LL
LU
UL
Spin OAM
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P-odd energy-momentum tensor
Chiral decomposition
General parametrization
Twist-2
Twist-3
[C.L. (2014)]
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Some figures
[C.L. (2014)]
Valence number
Spin and kinetic OAM of valence quarks are anti-correlated !
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Phase-space transverse modes
Parametrization of a correlator is not unique Natural modes ?
[C.L., Pasquini (in preparation)]
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Phase-space transverse modes
Parametrization of a correlator is not unique Natural modes ?
[C.L., Pasquini (in preparation)]
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Phase-space transverse modes
Properties under
parity and time-reversal
Parametrization of a correlator is not unique Natural modes ?
[C.L., Pasquini (in preparation)]
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Phase-space transverse modes
Unpolarized quark in unpolarized target
[C.L., Pasquini (in preparation)]
UU
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Phase-space transverse modes
Unpolarized quark in longitudinally polarized target
[C.L., Pasquini (in preparation)]
LU
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Phase-space transverse modes
Unpolarized quark in transversely polarized target (1)
[C.L., Pasquini (in preparation)]
TU
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Phase-space transverse modes
Unpolarized quark in transversely polarized target (2)
[C.L., Pasquini (in preparation)]
TU
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Phase-space transverse modes
Unpolarized quark in transversely polarized target (1+2)
[C.L., Pasquini (in preparation)]
TU
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Conclusions
• Complete characterization of spin structure requires spin-orbit correlation
• Like quark OAM, quark spin-orbit correlation is given by moments of measurable parton distributions
• Natural phase-space transverse modes help to understand the physics contained in parton distributions
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Backup slides
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Energy-momentum tensor
In presence of spin density
In rest frame
No « spin » contribution !
Belinfante « improvement »
Spin density gradient Four-momentum circulation
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Light-front quark models Wigner rotation
Light-front overlap representation
[C.L., Pasquini, Vanderhaeghen (2011)]
GTMDs ~
Momentum Polarization