On the stability of accelerating relativistic shock waves

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dc.creatorPalma, Giuseppe
dc.creatorVietri, Mario
dc.date2006-09-04
dc.date.accessioned2026-07-07T10:39:58Z
dc.date.available2026-07-07T10:39:58Z
dc.descriptionWe consider the corrugation instability of the self-similar flow with an accelerating shock in the highly relativistic regime. We derive the correct dispersion relation for the proper modes in the self-similar regime, and conclude that this solution is unstable.
dc.description25 pages, 10 figures. Accepted for publication in the Astrophysical Journal
dc.identifierhttps://arxiv.org/abs/astro-ph/0609074
dc.identifierhttp://arxiv.org/abs/astro-ph/0609074
dc.identifierAstrophys.J.653:1253-1265,2006
dc.identifierdoi:10.1086/508850
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181217
dc.subjectAstrophysics
dc.titleOn the stability of accelerating relativistic shock waves
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