Implications of CHOOZ results for the decoupling of solar and atmospheric neutrino oscillations
| dc.creator | Bilenky, S. M. | |
| dc.creator | Giunti, C. | |
| dc.date | 1998-02-02 | |
| dc.date | 1998-02-24 | |
| dc.date.accessioned | 2026-07-07T10:33:36Z | |
| dc.date.available | 2026-07-07T10:33:36Z | |
| dc.description | We have considered the results of solar and atmospheric neutrino oscillation experiments in the scheme of mixing of three neutrinos with a mass hierarchy. It is shown that the recent results of the CHOOZ experiment imply that |U_{e3}|^2<<1 (U is the neutrino mixing matrix), that the oscillations of solar neutrinos are described by the two-generation formalism and that the oscillations of solar and atmospheric neutrinos decouple. It is also shown that if not only |U_{e3}|^2<<1 but also |U_{e3}|<<1, then the oscillations of atmospheric neutrinos do not depend on matter effects and are described by the two-generation formalism. In this case, with an appropriate identification of the mixing parameters, the two-generation analyses of solar and atmospheric neutrino data provide direct information on the mixing parameters of three neutrinos. We discuss the possibility to get information on |U_{e3}|^2 in long-baseline neutrino oscillation experiments. | |
| dc.description | 12 pages, no figures | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9802201 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9802201 | |
| dc.identifier | Phys.Lett.B444:379-386,1998 | |
| dc.identifier | doi:10.1016/S0370-2693(98)01418-X | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/179174 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Implications of CHOOZ results for the decoupling of solar and atmospheric neutrino oscillations | |
| dc.type | text |