MSW Oscillations - LMA and Subdominant Effects
| dc.creator | Friedland, Alexander | |
| dc.date | 2006-12-20 | |
| dc.date.accessioned | 2026-07-07T07:40:27Z | |
| dc.date.available | 2026-07-07T07:40:27Z | |
| dc.description | New physics near the TeV scale could modify neutrino-matter interactions or generate a relatively large neutrino magnetic (transition) moment. Both types of effects have been discussed since the 1970's as alternatives to mass-induced neutrino flavor oscillations. Nowadays, the availability of high-statistics data makes it possible to turn the idea around and ask: How well do the simple mass-induced oscillations describe solar neutrinos? At what level are the above-mentioned nonstandard effects excluded? Can we use solar neutrinos to constrain physics beyond the Standard Model? These notes review the sensitivity of the present-day solar neutrino experiments to the nonstandard neutrino interactions and transition moment and outline progress that may be expected in the near future. Based on a talk given at the Neutrino 2006 conference. | |
| dc.description | 8 pages, 5 figures, based on talk given at Neutrino 2006 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0612266 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0612266 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/121781 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | MSW Oscillations - LMA and Subdominant Effects | |
| dc.type | text |