On the Status of Three-Neutrino Mixing
| dc.creator | Bilenky, S. M. | |
| dc.date | 2001-10-16 | |
| dc.date | 2001-10-17 | |
| dc.date.accessioned | 2026-07-07T03:45:34Z | |
| dc.date.available | 2026-07-07T03:45:34Z | |
| dc.description | All existing solar and atmospheric neutrino oscillation data are described by the standard two-neutrino formulas with neutrino mass squared differences that satisfy the hierarchy relation $Δm^{2}_{sol} \ll Δm^{2}_{atm}$. We discuss this phenomenon from the point of view of three-neutrino mixing. Possibilities to see effects of three-neutrino mixing and, in particular, effects of CP-violation in the lepton sector depend on the values of $|U_{e3}|^2 $ and $Δm^{2}_{sol}$. We present an upper bound of $|U_{e3}|^2 $, which was obtained from a three-neutrino analysis of CHOOZ data in the case if the solar neutrino oscillation parameters lie in the LMA allowed region. | |
| dc.description | 11 pages, Report at the Meeting NO-VE, Neutrino oscillations at Venice, 24-26 July 2001 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0110210 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0110210 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/40967 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | On the Status of Three-Neutrino Mixing | |
| dc.type | text |