Solar, Supernova, and Atmospheric Neutrinos

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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.
To be published in the Proceedings of the 1998 Australian National University Nuclear Physics Summer School; S. Kuyucak, Ed. 83 pages, 22 figures

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Nuclear Theory, Astrophysics, High Energy Physics - Phenomenology

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http://salesiana.dossiersoluciones.com/handle/123456789/83141

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/nucl-th/9903038
 http://arxiv.org/abs/nucl-th/9903038

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arXiv