Abstract
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.
Original language | English |
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Pages (from-to) | 379-383 |
Number of pages | 5 |
Journal | Astrophysics and Space Science |
Volume | 298 |
Issue number | 1-2 |
DOIs | |
Publication status | Published - Jun 2005 |
Event | 5th International Conference on High Energy Density Laboratory Astrophysics - Tucson, Azerbaijan Duration: 10 Mar 2004 → 13 Mar 2004 |