The importance of neutrino opacities for the accretion luminosity in spherically symmetric supernova models

Details The importance of neutrino opacities for the accretion luminosity in spherically symmetric supernova models The importance of neutrino opacities for the accretion luminosity in spherically symmetric supernova models

2002-03-15

arxiv.org/abs/astro-ph/0203260v1

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figures, to appear in W. Hillebrandt and E. Mueller, eds., Proceedings of the 11th Workshop on "Nuclear Astrophysic

Scientific paper

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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