Maximally-Mixed Three Generations of Neutrinos and the Solar and Atmospheric Neutrino Problems
| dc.creator | Kim, C. W. | |
| dc.creator | Lee, J. A. | |
| dc.date | 1993-11-19 | |
| dc.date.accessioned | 2026-07-07T03:56:36Z | |
| dc.date.available | 2026-07-07T03:56:36Z | |
| dc.description | Motivated by the indication that both the Solar and the atmospheric neutrino puzzles may simultaneously be solved by (vacuum as well as matter-induced resonant) oscillations of two generations of neutrinos with large mixing, we have analyzed the data on the Solar and atmospheric neutrinos assuming that all {\it three} neutrinos are maximally mixed. It is shown that the results of two-generation analyses are still valid even in the three-generation scheme, {\it i.e.}, the two puzzles can be solved simultaneously if $Δm_{21}^2 = m_2^2-m_1^2\simeq 10^{-10}\mbox{eV}^2$ and $Δm_{31}^2 = 10^{-3}\sim 10^{-1}\mbox{eV}^2$. We have also demonstrated explicitly that with the use of the see-saw mechanism it is possible to have large or maximal mixings for neutrinos even though their masses are highly non-degenerate. | |
| dc.description | 20pages, plain LaTeX, JHU-TIPAC-930023 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9311317 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9311317 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/45045 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Maximally-Mixed Three Generations of Neutrinos and the Solar and Atmospheric Neutrino Problems | |
| dc.type | text |