paper

Stability of Relativistic Blast Waves

arXiv:astro-ph/0002472 · doi:10.1143/PTP.103.549

Abstract

A spherical blast wave with relativistic velocity can be described by a similarity solution, that is used for theoretical models of gamma-ray bursts. We consider the linear stability of such a relativistic blast wave propagating into a medium with density gradient. The perturbation can also be expressed by a self-similar form. We show that the shock front is unstable in general, and we evaluate the growth rate.

11 pages, 2 figures, Accepted for publication in Prog.Theor. Phys