GUT Implications from Neutrino Mass
| dc.creator | Albright, Carl H. | |
| dc.date | 2001-06-14 | |
| dc.date.accessioned | 2026-07-07T11:31:06Z | |
| dc.date.available | 2026-07-07T11:31:06Z | |
| dc.description | An overview is given of the experimental neutrino mixing results and types of neutrino models proposed, with special attention to the general features of various GUT models involving intra-family symmetries and horizontal flavor symmetries. Many of the features are then illustrated by a specific SO(10) SUSY GUT model formulated by S.M. Barr and the author which can explain all four types of solar neutrino mixing solutions by various choices of the right-handed Majorana mass matrix. The quantitative nature of the model's large mixing angle solution is used to compare the reaches of a neutrino super beam and a neutrino factory for determining the small U_{e3} mixing matrix element. | |
| dc.description | 9 pages, 1 figure, invited talk at the NUFACT'01 Workshop in Tsukuba, Japan, 24-30 May 2001 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0106157 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0106157 | |
| dc.identifier | Nucl.Instrum.Meth.A503:47-52,2001 | |
| dc.identifier | doi:10.1016/S0168-9002(03)00640-5 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/197164 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | High Energy Physics - Experiment | |
| dc.title | GUT Implications from Neutrino Mass | |
| dc.type | text |