Universal quark-lepton mixing and determination of neutrino masses
| dc.creator | Osland, Per | |
| dc.creator | Wu, Tai Tsun | |
| dc.date | 2000-06-16 | |
| dc.date.accessioned | 2026-07-07T03:41:44Z | |
| dc.date.available | 2026-07-07T03:41:44Z | |
| dc.description | If three right-handed neutrinos are added to the Standard Model, then, for the three known generations, there are six quarks and six leptons. It is then natural to assume that the symmetry considerations that have been applied to the quark matrices are also valid for the lepton mass matrices. Under this assumption, the solar and atmospheric neutrino data can be used to determine the individual neutrino masses. Three minima have been found, using the chi^2 fit, and, from these minima, it is determined that the mass of the lightest neutrino is 1.3\times10^-3 eV, that of the next heavier neutrino is 1.3\times10^-2 eV, while the mass of the heaviest neutrino is 3.4\times10^-2, 5.8\times10^-2 or 9.4\times10^-2 eV. | |
| dc.description | 10 pages | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0006185 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0006185 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/39683 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Universal quark-lepton mixing and determination of neutrino masses | |
| dc.type | text |