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

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dc.creatorLiebendoerfer, M.
dc.creatorMesser, O. E. B.
dc.creatorMezzacappa, A.
dc.creatorHix, W. R.
dc.creatorThielemann, F. -K.
dc.creatorLanganke, K.
dc.date2002-03-15
dc.date.accessioned2026-07-07T02:03:09Z
dc.date.available2026-07-07T02:03:09Z
dc.descriptionBased 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).
dc.description4 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
dc.identifierhttps://arxiv.org/abs/astro-ph/0203260
dc.identifierhttp://arxiv.org/abs/astro-ph/0203260
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4287
dc.subjectAstrophysics
dc.titleThe importance of neutrino opacities for the accretion luminosity in spherically symmetric supernova models
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