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Relativistic Spin Magnetohydrodynamics

Samapan Bhadury, Wojciech Florkowski, Amaresh Jaiswal, Avdhesh Kumar, Radosław Ryblewski

2022Physical Review Letters67 citationsDOIOpen Access PDF

Abstract

Starting from the kinetic theory description of massive spin-1/2 particles in the presence of a magnetic field, equations for relativistic dissipative nonresistive 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 nonequilibrium 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 Haas 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 the hydrodynamic equation.

Topics & Concepts

PhysicsBoltzmann equationDistribution functionDissipative systemMagnetohydrodynamicsMagnetic fieldNon-equilibrium thermodynamicsPhase spaceSpin (aerodynamics)Relaxation (psychology)Quantum electrodynamicsClassical mechanicsQuantum mechanicsSocial psychologyThermodynamicsPsychologyHigh-Energy Particle Collisions ResearchGas Dynamics and Kinetic TheoryHigh-pressure geophysics and materials
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