Neutrino Mass in Physics and Astrophysics

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dc.creatorWolfenstein, Lincoln
dc.date1996-04-23
dc.date.accessioned2026-07-07T11:14:37Z
dc.date.available2026-07-07T11:14:37Z
dc.descriptionThe symmetry between quarks and leptons suggests that neutrinos should have mass. As embodied in the grand unified theory SO(10) this yields masses that can only be detected by neutrino oscillations. Such oscillations could be very important for supernova physics. Present observations of solar neutrinos when combined with standard solar model calculations imply particular parameters for neutrino masses and mixings. If the solar model is somewhat relaxed quite different possibilities emerge, which yield very different predictions for future experiments.
dc.identifierhttps://arxiv.org/abs/hep-ph/9604389
dc.identifierhttp://arxiv.org/abs/hep-ph/9604389
dc.identifierContemp.Phys.37:175-182,1996
dc.identifierdoi:10.1080/00107519608217526
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/192133
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNeutrino Mass in Physics and Astrophysics
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