Neutrino Masses in Astrophysics and Cosmology
| dc.creator | Raffelt, Georg G. | |
| dc.date | 1997-04-14 | |
| dc.date.accessioned | 2026-07-07T04:01:32Z | |
| dc.date.available | 2026-07-07T04:01:32Z | |
| dc.description | Astrophysical and cosmological arguments and observations give us the most restrictive constraints on neutrino masses, electromagnetic couplings, and other properties. Conversely, massive neutrinos would contribute to the cosmic dark-matter density and would play an important role for the formation of structure in the universe. Neutrino oscillations may well solve the solar neutrino problem, and can have a significant impact on supernova physics. | |
| dc.description | 11 pages, REVTEX, figures embedded. Minor update of my contribution to the Proceedings of the Summer School on Physics with Neutrinos (Zuoz, Switzerland, August 4-10, 1996), ed. by M.P.Locher (PSI, Villingen, 1996) | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9704315 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9704315 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/46928 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Neutrino Masses in Astrophysics and Cosmology | |
| dc.type | text |