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Effects of rotation and acceleration in the axial current: density operator vs Wigner function

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arxiv 1807.03584 v1 pith:OIQYLXLD submitted 2018-07-10 hep-th

Effects of rotation and acceleration in the axial current: density operator vs Wigner function

classification hep-th
keywords accelerationaxialcurrentdensityeffectsoperatorvorticitycoefficients
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The hydrodynamic coefficients in the axial current are calculated on the basis of the equilibrium quantum statistical density operator in the third order of perturbation theory in thermal vorticity tensor both for the case of massive and massless fermions. The coefficients obtained describe third-order corrections to the Chiral Vortical Effect and include the contribution from local acceleration. We show that the methods of the Wigner function and the statistical density operator lead to the same result for an axial current in describing effects associated only with vorticity when the local acceleration is zero, but differ in describing mixed effects for which both acceleration and vorticity are significant simultaneously.

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Cited by 2 Pith papers

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    A local pressure for rotating massless fermions is proposed that satisfies both the Euler relation and the thermodynamic differential relations, resolving a known spin-hydrodynamics tension.