Discrete Self Similarity in Filled Type I Strong Explosions

Abstract

We present new solutions to the strong explosion problem in a non power law density profi{}le. The unperturbed self similar solutions developed by Sedov, Taylor and Von Neumann describe strong Newtonian shocks propagating into a cold gas with a density profile falling off as $r^{-\omega }$, where $\omega \le \frac{7-\gamma }{\gamma +1}$ (filled type I solutions), and $\gamma$ is the adiabatic index of the gas. The perturbations we consider are spherically symmetric and log periodic with respect to the radius. While the unperturbed solutions are continuously self similar, the log periodicity of the density perturbations leads to a discrete self similarity of the perturbations, i.e., the solution repeats itself up to a scaling at discrete time intervals. We discuss these solutions and verify them against numerical integrations of the time dependent hydrodynamic equations. This is an extension of a previous investigation on type II solutions and helps clarifying boundary conditions for perturbations to type I self similar solutions.

References in corpus (3)

• PLUTO: a Numerical Code for Computational Astrophysics
• Explosion Mechanisms of Core-Collapse Supernovae
• Discrete Self-Similarity in Type-II Strong Explosions

Cited by in corpus (1)

• Angular Density Perturbations to Filled Type I Strong Explosions