1999/03/13 by A. B. Balantekin, Balantekin, A. B., W. C. Haxton +1
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Nuclear Theory (nucl-th) #astro-ph #hep-ph #nucl-th
paper · pdf · doi:10.48550/arxiv.nucl-th/9903038
To be published in the Proceedings of the 1998 Australian National University Nuclear Physics Summer School; S. Kuyucak, Ed. 83 pages, 22 figures
arxiv created 1999/03/13 · arxiv updated 2009/11/30
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.