Solar, Supernova, and Atmospheric Neutrinos

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dc.creatorBalantekin, A. B.
dc.creatorHaxton, W. C.
dc.date1999-03-13
dc.date.accessioned2026-07-07T05:42:59Z
dc.date.available2026-07-07T05:42:59Z
dc.descriptionIn these Canberra summer school lectures we treat a number of topical issues in neutrino astrophysics: the solar neutrino problem, including the physics of the standard solar model, helioseismology, and the possibility that the solution involves new particle physics; atmospheric neutrinos; Dirac and Majorana neutrino masses and their consequences for low-energy weak interactions; red giant evolution as a test of new particle astrophysics; the supernova mechanism; spin-flavor oscillations and oscillations into sterile states, including the effects of density fluctuations; and neutrino-induced and explosive nucleosynthesis.
dc.descriptionTo be published in the Proceedings of the 1998 Australian National University Nuclear Physics Summer School; S. Kuyucak, Ed. 83 pages, 22 figures
dc.identifierhttps://arxiv.org/abs/nucl-th/9903038
dc.identifierhttp://arxiv.org/abs/nucl-th/9903038
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/83141
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSolar, Supernova, and Atmospheric Neutrinos
dc.typetext

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