Solar, Supernova, and Atmospheric Neutrinos

Details Solar, Supernova, and Atmospheric Neutrinos Solar, Supernova, and Atmospheric Neutrinos

1999-03-13

arxiv.org/abs/nucl-th/9903038v1

Physics

Nuclear Physics

Nuclear Theory

To be published in the Proceedings of the 1998 Australian National University Nuclear Physics Summer School; S. Kuyucak, Ed. 8

Scientific paper

In 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.

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