Name
Abstract | ||
|---|---|---|
We present preliminary results from multidimensional numerical studies of pair-instability supernova (PSN), studying the fluid instabilities that occur in multiple spatial dimensions. We use the new radiation-hydrodynamics code, CASTRO, and introduce a new mapping procedure that defines the initial conditions for the multidimensional runs in such a way that conservation of physical quantities is guaranteed at any level of resolution. |
Year | DOI | Venue |
|---|---|---|
2011 | 10.1016/j.cpc.2010.06.032 | Computer Physics Communications |
Keywords | Field | DocType |
Stellar evolution,Massive star,Pair-instability supernovae | Statistical physics,Supernova,Astrophysics,Physical quantity,Pair-instability supernova,Mathematical analysis,Instability,Physics,Stellar evolution | Journal |
Volume | Issue | ISSN |
182 | 1 | 0010-4655 |
Citations | PageRank | References |
0 | 0.34 | 0 |
Authors | ||
3 | ||
Name | Order | Citations | PageRank |
|---|---|---|---|
| Ke-Jung Chen | 1 | 0 | 0.34 |
| Alexander Heger | 2 | 0 | 0.34 |
| Ann S. Almgren | 3 | 82 | 22.33 |