The Physics of Core-Collapse Supernova Explosions
Abstract
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.
Cite
@article{arxiv.astro-ph/9506060,
title = {The Physics of Core-Collapse Supernova Explosions},
author = {Adam Burrows anbd John Hayes},
journal= {arXiv preprint arXiv:astro-ph/9506060},
year = {2007}
}
Comments
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