Dispersion relations of relativistic radiation hydrodynamics

Fuente: arXiv
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Auteur principal: Gavassino, Lorenzo
Format: Preprint
Publié: 2024
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author Gavassino, Lorenzo
author_facet Gavassino, Lorenzo
contents We compute the linearised dispersion relations of shear waves, heat waves, and sound waves in relativistic ''matter+radiation'' fluids with grey absorption opacities. This is done by solving radiation hydrodynamics perturbatively in the ratio ''radiation stress-energy''/''matter stress-energy''. The resulting expressions $ω\, {=} \, ω(k)$ accurately describe the hydrodynamic evolution for any $k\, {\in}\, \mathbb{R}$. General features of the dynamics (e.g., covariant stability, propagation speeds, and damping of discontinuities) are argued directly from the analytic form of these dispersion relations.
format Preprint
id arxiv_https___arxiv_org_abs_2412_00275
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Dispersion relations of relativistic radiation hydrodynamics
Gavassino, Lorenzo
High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
Nuclear Theory
We compute the linearised dispersion relations of shear waves, heat waves, and sound waves in relativistic ''matter+radiation'' fluids with grey absorption opacities. This is done by solving radiation hydrodynamics perturbatively in the ratio ''radiation stress-energy''/''matter stress-energy''. The resulting expressions $ω\, {=} \, ω(k)$ accurately describe the hydrodynamic evolution for any $k\, {\in}\, \mathbb{R}$. General features of the dynamics (e.g., covariant stability, propagation speeds, and damping of discontinuities) are argued directly from the analytic form of these dispersion relations.
title Dispersion relations of relativistic radiation hydrodynamics
topic High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
Nuclear Theory
url https://arxiv.org/abs/2412.00275