From CKM Matrix to MNS Matrix: A Model Based on Supersymmetric $SO(10) \times U(2)_{F}$ Symmetry

Details From CKM Matrix to MNS Matrix: A Model Based on Supersymmetric $SO(10) \times U(2)_{F}$ Symmetry From CKM Matrix to MNS Matrix: A Model Based on Supersymmetric $SO(10) \times U(2)_{F}$ Symmetry

2000-05-29

arxiv.org/abs/hep-ph/0005292v3

Phys.Rev.D62:113007,2000

Physics

High Energy Physics

High Energy Physics - Phenomenology

9 pages; REVTex; no figures; version to appear in Phys. Rev. D

Scientific paper

10.1103/PhysRevD.62.113007

We construct a realistic model based on SUSY SO(10) with U(2) flavor symmetry. In contrast to the commonly used effective operator approach, $126-$dimensional Higgses are used to construct the Yukawa sector. R-parity symmetry is thus preserved at low energies. The Dirac and right-handed Majorana mass matrices in our model have very small mixing, and they combine with the seesaw mechanism resulting in a large leptonic mixing. The symmetric mass textures arising from the left-right symmetry breaking chain of SO(10) give rise to very good predictions; 15 masses (including 3 right-handed Majorana neutrino 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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