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Causality in dissipative relativistic magnetohydrodynamics

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arxiv 2411.04966 v1 pith:65ZCVCKF submitted 2024-11-07 hep-th gr-qchep-ph

classification hep-thgr-qchep-ph
keywords causalitydissipativerelativistictheoryanalysisfluidlinearizedmagnetohydrodynamics
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We explore the relationship between linear and non-linear causality in theories of dissipative relativistic fluid dynamics. While for some fluid-dynamical theories, a linearized causality analysis can be used to determine whether the full non-linear theory is causal, for others it can not. As an illustration, we study relativistic viscous magnetohydrodynamics supplemented by a neutral-particle current, with resistive corrections to the conservation of magnetic flux. The dissipative theory has 10 transport coefficients, including anisotropic viscosities, electric resistivities, and neutral-particle conductivities. We show how causality properties of this magnetohydrodynamic theory, in the most general fluid frame, may be understood from the linearized analysis.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Causality constraints and anisotropic states

    hep-th 2025-12 conditional novelty 7.0 of 10

    In anisotropic relativistic fluids, branch-point dispersion relations force a continuum of complex-wavevector mode collisions, and causality bounds the convergence radius direction-by-direction in terms of transport c...

  2. Perturbations of relativistic dissipative stars

    gr-qc 2024-11 conditional novelty 7.0 of 10

    Linearized perturbations of relativistic stars with BDNK viscosity reduce to two coupled wave equations in the axial sector and five coupled wave equations plus a constraint in the polar sector, including a new viscous mode.

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