2019
DOI: 10.1016/j.physletb.2019.05.040
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Fate of spin polarization in a relativistic fluid: An entropy-current analysis

Abstract: We derive relativistic hydrodynamic equations with a dynamical spin degree of freedom on the basis of an entropy-current analysis. The first and second laws of local thermodynamics constrain possible structures of the constitutive relations including a spin current and the antisymmetric part of the (canonical) energy-momentum tensor. Solving the obtained hydrodynamic equations within the linear-mode analysis, we find spin-diffusion modes, indicating that spin density is damped out after a characteristic time s… Show more

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Cited by 187 publications
(194 citation statements)
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“…This suggests that if the spin is (quasi-)conserved, after polarized in the early stage by the OAM, the pressure gradient would be possibly drive a similar φ p dependence as that for the T-vorticity. This may be verified by the simulation using spin hydrodynamics [73,75].…”
Section: Discussionmentioning
confidence: 65%
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“…This suggests that if the spin is (quasi-)conserved, after polarized in the early stage by the OAM, the pressure gradient would be possibly drive a similar φ p dependence as that for the T-vorticity. This may be verified by the simulation using spin hydrodynamics [73,75].…”
Section: Discussionmentioning
confidence: 65%
“…In relativistic hydrodynamics, in order to obtain the spin vector, we need to first obtain T , u µ , and Ω µν by solving the hydrodynamic equations in which the spin degree of freedom (or equivalently Ω µν ) is treated on the same footing as T and u µ . Such a framework is the spin hydrodynamics [73,75]. However, the numerical spin hydrodynamics has not been established yet.…”
Section: Spin Polarization and Vorticitymentioning
confidence: 99%
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