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

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

2000-09-05

arxiv.org/abs/hep-ph/0009059v1

Osaka 2000, High energy physics, vol. 2, 1051-1053.

Physics

High Energy Physics

High Energy Physics - Phenomenology

3 pages; talks presented at ICHEP2000 and DPF2000

Scientific paper

We 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.

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