Neutrino Mixing from the CKM matrix in SUSY SO(10) × U(2)_F

2000/09/05 by Mu-Chun Chen, K. T. Mahanthappa
Physics and Astronomy · #hep-ph

paper · pdf

published as Osaka 2000, High energy physics, vol. 2, 1051-1053. · 3 pages; talks presented at ICHEP2000 and DPF2000

arxiv created 2000/09/05 · arxiv updated 2009/11/30

Abstract

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.

Related

• Predictive SUSY SO(10) X Delta (48) X U(1) Model for CP Violation, Neutrino Oscillation, Fermion Masses and Mixings with Small tan(beta)
• Predictive SUSY GUT Model for CP Violation, Fermion Masses and Mixings
• Masses and mixing of neutrinos in grand unified SO(10) model
• Bi-maximal Neutrino Mixing And Anomalous Flavor \cal U(1)
• Low Energy Phenomena in a Model With Symmetry Group SUSY SO(10) X Delta (48) X U(1)