Supernova neutrinos, from back of the envelope to supercomputer

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dc.creatorCardall, Christian Y.
dc.date2007-01-29
dc.date.accessioned2026-07-07T07:43:25Z
dc.date.available2026-07-07T07:43:25Z
dc.descriptionWhile an understanding of supernova explosions will require sophisticated large-scale simulations, it is nevertheless possible to outline the most basic features of the neutrino emission resulting from stellar core collapse with a pedestrian account that, through reliance upon broadly accessible physical ideas, remains simple and largely self-contained.
dc.description7 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0701831
dc.identifierhttp://arxiv.org/abs/astro-ph/0701831
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/122819
dc.subjectAstrophysics
dc.titleSupernova neutrinos, from back of the envelope to supercomputer
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