Relativistic Spin Magnetohydrodynamics
Samapan Bhadury, Wojciech Florkowski, Amaresh Jaiswal, Avdhesh Kumar, and Radoslaw Ryblewski

TL;DR
This paper develops a relativistic spin magnetohydrodynamics framework starting from kinetic theory, revealing new spin-magnetic coupling effects and deriving related transport coefficients.
Contribution
It introduces a novel relativistic dissipative magnetohydrodynamics model incorporating spin effects, including the first derivation of spin-magnetic coupling at gradient order.
Findings
Emergence of Einstein-de Hass and Barnett effects from the framework.
Calculation of multiple transport coefficients involving spin and magnetic field.
Identification of spin-magnetic coupling appearing at gradient order in hydrodynamics.
Abstract
Starting from kinetic theory description of massive spin-1/2 particles in presence of magnetic field, equations for relativistic dissipative non-resistive magnetohydrodynamics are obtained in the small polarization limit. We use a relaxation time approximation for the collision kernel in the relativistic Boltzmann equation and calculate non-equilibrium corrections to the phase-space distribution function of spin-polarizable particles. We demonstrate that our framework naturally leads to emergence of the well known Einstein-de Hass and Barnett effects. We obtain multiple transport coefficients and show, for the first time, that the coupling between spin and magnetic field appear at gradient order in hydrodynamic equations.
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Taxonomy
TopicsGas Dynamics and Kinetic Theory · High-Energy Particle Collisions Research · Fluid Dynamics and Turbulent Flows
