Neutrino Unification
| dc.creator | Chankowski, P. H. | |
| dc.creator | Ioannisian, A. | |
| dc.creator | Pokorski, S. | |
| dc.creator | Valle, J. W. F | |
| dc.date | 2000-11-10 | |
| dc.date | 2001-02-14 | |
| dc.date.accessioned | 2026-07-07T11:09:05Z | |
| dc.date.available | 2026-07-07T11:09:05Z | |
| dc.description | Present neutrino data are consistent with neutrino masses arising from a common seed at some ``neutrino unification'' scale $M_X$. Such a simple theoretical ansatz naturally leads to quasi-degenerate neutrinos that could lie in the electron-volt range with neutrino mass splittings induced by renormalization effects associated with supersymmetric thresholds. In such a scheme the leptonic analogue of the Cabibbo angle $θ_{\odot}$ describing solar neutrino oscillations is nearly maximal. Its exact value is correlated with the smallness of $θ_{reactor}$. These features agree both with latest data on the solar neutrino spectra and with the reactor neutrino data. The two leading mass-eigenstate neutrinos present in \ne form a pseudo-Dirac neutrino, avoiding conflict with neutrinoless double beta decay. | |
| dc.description | RevTex format, 2 figures, 4 pages, a few new references, no other important change, figures unchanged, version to be published in PRL | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0011150 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0011150 | |
| dc.identifier | Phys.Rev.Lett.86:3488-3491,2001 | |
| dc.identifier | doi:10.1103/PhysRevLett.86.3488 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/190347 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Neutrino Unification | |
| dc.type | text |