Core-collapse supernova simulations: Variations of the input physics

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dc.creatorRampp, M.
dc.creatorBuras, R.
dc.creatorJanka, H. -Th.
dc.creatorRaffelt, G.
dc.date2002-03-27
dc.date.accessioned2026-07-07T02:03:17Z
dc.date.available2026-07-07T02:03:17Z
dc.descriptionSpherically symmetric simulations of stellar core collapse and post-bounce evolution are used to test the sensitivity of the supernova dynamics to different variations of the input physics. We consider a state-of-the-art description of the neutrino-nucleon interactions, possible lepton-number changing neutrino reactions in the neutron star, and the potential impact of hydrodynamic mixing behind the supernova shock.
dc.description6 pages, 6 ps figures (in color), to appear in W. Hillebrandt and E. Mueller, eds., Proceedings of the 11th Workshop on "Nuclear Astrophysics" held at Ringberg Castle, February 11-16, 2002
dc.identifierhttps://arxiv.org/abs/astro-ph/0203493
dc.identifierhttp://arxiv.org/abs/astro-ph/0203493
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4331
dc.subjectAstrophysics
dc.titleCore-collapse supernova simulations: Variations of the input physics
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