The importance of neutrino opacities for the accretion luminosity in spherically symmetric supernova models
M. Liebendoerfer, O. E. B. Messer, A. Mezzacappa, W. R. Hix, F. -K. Thielemann, K. Langanke
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).
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