We consider the corrugation instability of a 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.
On the stability of accelerating relativistic shock waves
Palma Giuseppe;
2006
Abstract
We consider the corrugation instability of a 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.File in questo prodotto:
Non ci sono file associati a questo prodotto.
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
