The importance of neutrino opacities for the accretion luminosity in spherically symmetric supernova models
arXiv:astro-ph/0203260
Abstract
Based on general relativistic three-flavor Boltzmann neutrino transport, we compare simulations of the postbounce evolution for five different stellar progenitors with 13 and 20 solar masses (Nomoto & Hashimoto '88), and 15, 25, and 40 solar masses (Woosley & Weaver '95).
4 pages, 3 figures, to appear in W. Hillebrandt and E. Mueller, eds., Proceedings of the 11th Workshop on "Nuclear Astrophysics" held at Rinberg Castle, February 11-16, 2002