On the stability of accelerating relativistic shock waves

Details On the stability of accelerating relativistic shock waves On the stability of accelerating relativistic shock waves

2006-09-04

arxiv.org/abs/astro-ph/0609074v1

Astrophys.J.653:1253-1265,2006

Astronomy and Astrophysics

Astrophysics

25 pages, 10 figures. Accepted for publication in the Astrophysical Journal

Scientific paper

10.1086/508850

We 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.

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