Massive neutrinos and lepton-flavour-violating processes
| dc.creator | Casas, J. A. | |
| dc.creator | Ibarra, A. | |
| dc.date | 2001-09-18 | |
| dc.date.accessioned | 2026-07-07T03:45:18Z | |
| dc.date.available | 2026-07-07T03:45:18Z | |
| dc.description | If neutrino masses and mixings are suitable to explain the atmospheric and solar neutrino fluxes, this amounts to contributions to FCNC processes, in particular $μ\to e, γ$. If the theory is supersymmetric and the origin of the masses is a see-saw mechanism, we show that the prediction for BR($μ\to e, γ$) is in general larger than the experimental upper bound, especially if the solar data are explained by a large angle MSW effect, which recent analyses suggest as the preferred scenario. | |
| dc.description | 10 pages, 3 figures, Talk given at Cairo International Conference on High Energy Physics, Cairo (CICHEP 2001), Egypt, 9-14, January 2001 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0109161 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0109161 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/40882 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Massive neutrinos and lepton-flavour-violating processes | |
| dc.type | text |