A Supersymmetric Solution to the Solar and Atmospheric Neutrino Anomalies
| dc.creator | Brooijmans, G. | |
| dc.date | 1998-08-31 | |
| dc.date | 1998-11-23 | |
| dc.date.accessioned | 2026-07-07T04:04:40Z | |
| dc.date.available | 2026-07-07T04:04:40Z | |
| dc.description | The formalism for neutrino flavor change induced by lepton family number violating interactions is developed for the three-neutrino case, and used to derive the corresponding flavor change probabilities in matter. Applied to the solar and atmospheric neutrino fluxes, it is argued that the observed anomalies, including the zenith dependence for the atmospheric case, could be due to such interactions. | |
| dc.description | 6 pages, 1 figure Modifications: include limit from tau -> rho mu (leads to somewhat different conclusions) and a change to the figure | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9808498 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9808498 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/48189 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | A Supersymmetric Solution to the Solar and Atmospheric Neutrino Anomalies | |
| dc.type | text |