Causality and stability in relativistic viscous non-resistive magneto-fluid dynamics
Rajesh Biswas, Ashutosh Dash, Najmul Haque, Shi Pu, Victor Roy

TL;DR
This paper analyzes the causality and stability of relativistic viscous magneto-hydrodynamics, incorporating magnetic field effects into Israel-Stewart theory, and finds conditions under which the fluid remains stable and causal.
Contribution
It introduces a modified Israel-Stewart theory including magnetic effects and examines how magnetic fields influence causality and stability in relativistic viscous fluids.
Findings
Causality bounds are independent of magnetic field magnitude for bulk viscosity.
Modified IS theory reveals new non-hydrodynamic modes with preserved causality conditions.
Fluid remains stable and causal under certain asymptotic conditions despite magnetic influences.
Abstract
We investigate the causality and the stability of the relativistic viscous magneto-hydrodynamics in the framework of the Israel-Stewart (IS) second-order theory, and also within a modified IS theory which incorporates the effect of magnetic fields in the relaxation equations of the viscous stress. We compute the dispersion relation by perturbing the fluid variables around their equilibrium values. In the ideal magnetohydrodynamics limit, the linear dispersion relation yields the well-known propagating modes: the Alfv\'en and the magneto-sonic modes.In the presence of bulk viscous pressure, the causality bound is found to be independent of the magnitude of the magnetic field. The same bound also remains true, when we take the full non-linear form of the equation using the method of characteristics. In the presence of shear viscous pressure, the causality bound is independent of the…
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