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Fluctuation and Dissipation of Axial Charge from Massive Quarks

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arxiv 1712.08429 v2 pith:YW4LKT7J submitted 2017-12-22 hep-ph nucl-th

classification hep-phnucl-th
keywords axialchargedissipationfluctuationmassquarkfindfree
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In quantum chromodynamics (QCD), axial charge is known to be non-conserved due to chiral anomaly and non-vanishing quark mass. In this paper, we explore the role of quark mass in axial charge fluctuation and dissipation. We present two separate calculations of axial charge correlator, which describe dynamics of axial charge. The first is free quarks at finite temperature. We find that axial charge can be generated through effective quantum fluctuations in free theory. However the fluctuation does not follow a random walk behavior. Due to the presence of axial symmetry breaking mass term, the axial charge also does not settle asymptotically to the thermodynamic limit given by susceptibility. The second calculation is in weakly coupled quark gluon plasma (QGP). We find in the hard thermal loop (HTL) approximation, the quark-gluon interaction leads to random walk growth of axial charge, but dissipation is not visible. We estimate relaxation time scale for axial charge, finding it lies beyond the HTL regime.

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  1. Schwinger-Keldysh effective action for hydrodynamics with approximate symmetries

    hep-th 2024-11 conditional novelty 6.0 of 10

    The axial charge relaxation coefficient in the Schwinger-Keldysh effective theory of QCD must be of second order in the quark mass, Γ_A = γ_A m_q^2, subleading in the broken phase and leading in the restored phase.

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