Core-Collapse Supernovae: Modeling between Pragmatism and Perfectionism

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dc.creatorJanka, H. -Th.
dc.creatorBuras, R.
dc.creatorJoyanes, F. S. Kitaura
dc.creatorMarek, A.
dc.creatorRampp, M.
dc.date2004-05-14
dc.date.accessioned2026-07-07T02:13:12Z
dc.date.available2026-07-07T02:13:12Z
dc.descriptionWe briefly summarize recent efforts in Garching for modeling stellar core collapse and post-bounce evolution in one and two dimensions. The transport of neutrinos of all flavors is treated by iteratively solving the coupled system of frequency-dependent moment equations together with a model Boltzmann equation which provides the closure. A variety of progenitor stars, different nuclear equations of state, stellar rotation, and global asymmetries due to large-mode hydrodynamic instabilities have been investigated to ascertain the road to finally successful, convectively supported neutrino-driven explosions.
dc.description8 pages, contribution to Procs. 12th Workshop on Nuclear Astrophysics, Ringberg Castle, March 22-27, 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0405289
dc.identifierhttp://arxiv.org/abs/astro-ph/0405289
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7733
dc.subjectAstrophysics
dc.titleCore-Collapse Supernovae: Modeling between Pragmatism and Perfectionism
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