Semi-Classical Spin Hydrodynamics in Flat and Curved Spacetime: Covariance, Linear Waves, and Bjorken Background
Annamaria Chiarini, Julia Sammet, and Masoud Shokri

TL;DR
This paper develops a covariant semi-classical spin hydrodynamics framework applicable to flat and curved spacetimes, analyzing linear wave modes, stability, and spin relaxation in various backgrounds, including Bjorken flow.
Contribution
It introduces covariant definitions, revises pseudo-gauge transformations, and derives linearized equations for semi-classical spin hydrodynamics, highlighting spin-fluid mode decoupling and spin relaxation effects.
Findings
Spin and fluid modes decouple linearly.
Spin wave damping depends only on spin relaxation time.
Limitations of Gibbs stability at first order in 1.
Abstract
We explore various aspects of semi-classical spin hydrodynamics, where hydrodynamic currents are derived from an expansion in the reduced Planck constant , incorporating both flat and curved spacetimes. After establishing covariant definitions for angular momentum currents, we demonstrate that the conservation of the energy-momentum tensor requires modifications involving the Riemann curvature and the spin tensors. We also revise pseudo-gauge transformations to ensure their applicability in curved spacetimes. Key assumptions for semi-classical spin hydrodynamics are introduced, enabling studies without explicitly invoking quantum kinetic theory. We derive and analyze the linearized semi-classical spin hydrodynamic equations, proving that spin and fluid modes decouple in the linear regime. As a concrete example, we study the ideal-spin approximation in a dissipative fluid with…
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