Toward a Standard Model of Core Collapse Supernovae
arXiv:astro-ph/0010580 · doi:10.1016/S0375-9474(01)00690-X
Abstract
In this paper, we discuss the current status of core collapse supernova models and the future developments needed to achieve significant advances in understanding the supernova mechanism and supernova phenomenology, i.e., in developing a supernova standard model.
To appear in Nuclear Physics A, in the proceedings of Nuclei in the Cosmos 2000, University of Aarhus, Aarhus, Denmark, June 27-July 1, 2000