We report analytical and numerical solutions describing the evolution of the coherent structure of bubbles and spikes in the Richtmyer-Meshkov instability in supernovae. It is shown that the dynamics of the flow is essentially non-local, and the nonlinear Richtmyer-Meshkov bubble flattens and decelerates.
|Number of pages||5|
|Journal||Astrophysics and Space Science|
|Publication status||Published - Jun 2005|
|Event||5th International Conference on High Energy Density Laboratory Astrophysics - Tucson, Azerbaijan|
Duration: 10 Mar 2004 → 13 Mar 2004