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 (US) |
|---|---|
| Pages (from-to) | 379-383 |
| Number of pages | 5 |
| Journal | Astrophysics and Space Science |
| Volume | 298 |
| Issue number | 1-2 |
| DOIs | |
| State | Published - Jun 1 2005 |
| Externally published | Yes |
Keywords
- Non-local
- Richtmyer-Meshkov
- Singularities
- Supernovae
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science