Neutrino Mixing from the CKM matrix in SUSY SO(10) \times U(2)_{F}

dc.creatorChen, Mu-Chun
dc.creatorMahanthappa, K. T.
dc.date2000-09-05
dc.date.accessioned2026-07-07T03:42:30Z
dc.date.available2026-07-07T03:42:30Z
dc.descriptionWe construct a realistic model based on SUSY SO(10) with U(2) flavor symmetry. A set of symmetric mass textures give rise to very good predictions; 15 masses and 6 mixing angles are predicted by 11 parameters. Both the vacuum oscillation and LOW solutions are favored for the solar neutrino problem.
dc.description3 pages; talks presented at ICHEP2000 and DPF2000
dc.identifierhttps://arxiv.org/abs/hep-ph/0009059
dc.identifierhttp://arxiv.org/abs/hep-ph/0009059
dc.identifierOsaka 2000, High energy physics, vol. 2, 1051-1053.
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/39920
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNeutrino Mixing from the CKM matrix in SUSY SO(10) \times U(2)_{F}
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