Viscous Flows and Conditions for Existence of Shocks in Relativistic Magnetic Hydrodynamics

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dc.creatorZhdanov, V. I.
dc.creatorTytarenko, P. V.
dc.creatorBorshch, M. S.
dc.date2004-07-23
dc.date.accessioned2026-07-07T02:14:07Z
dc.date.available2026-07-07T02:14:07Z
dc.descriptionWe present a criterion for a shock wave existence in relativistic magnetic hydrodynamics with an arbitrary (possibly non-convex) equation of state. The criterion has the form of algebraic inequality that involves equation of state of the fluid; it singles out the physical solutions and it can be easily checked for any discontinuity satisfying concervation laws. The method of proof uses introduction of small viscosity into the coupled set of equations of motion of ideal relativistic fluid with infinite conductivity and Maxwell equations.
dc.descriptionTalk presented at the International Workshop "Frontiers of Particle Astrophysics", Kiev, Ukraine, June 21-24, 2004. 10 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0407510
dc.identifierhttp://arxiv.org/abs/astro-ph/0407510
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7992
dc.subjectAstrophysics
dc.titleViscous Flows and Conditions for Existence of Shocks in Relativistic Magnetic Hydrodynamics
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