The Physics of Core-Collapse Supernova Explosions
| dc.creator | Hayes, Adam Burrows anbd John | |
| dc.date | 1995-06-08 | |
| dc.date.accessioned | 2026-07-07T02:19:51Z | |
| dc.date.available | 2026-07-07T02:19:51Z | |
| dc.description | Fresh insights and powerful numerical tools are revitalizing the theoretical exploration of the supernova mechanism. The realization that the protoneutron star is Rayleigh-Taylor unstable at various times and radii and, hence, that a multi-dimensional perspective is required is one agent of this revolution. However, a new physical understanding of the nature of explosions (even spherical explosions) that are driven by neutrino heating and that escape from deep within a gravitational potential well is also emerging. This, together with the new multi-dimensional approach, promises to establish a paradigm within which supernova explosions and their consequences can be studied in the future. | |
| dc.description | 7 pages, LateX, 3 Figures (best gotten from author), text and Table 1 to be LaTeX'ed separately, to be published in the proceedings of the 17'th Texas Symposium on Relativistic Astrophysics | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9506060 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9506060 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10030 | |
| dc.subject | Astrophysics | |
| dc.title | The Physics of Core-Collapse Supernova Explosions | |
| dc.type | text |