Quark-Lepton Mass Matrices with Flavor Symmetry
arXiv:hep-ph/9901210 · doi:10.1016/S0370-2693(99)00467-0
Abstract
The U(1) flavor symmetry explains the large mixing of neutrinos while it leads to the unique texture for the quark mass matrices. It is remarked that U(1) symmetric mass matrices have the phenomenological defects. In the quark sector, the mixing is predicted to be large compared with the expected value at the GUT scale. In the lepton sector, U(1) charges, which give a large mixing in the neutrino sector, also lead to the large one in the charged lepton sector. In the viewpoint of the flavor symmetry, this is an unpleasant feature because the neutrino mass hierarchy is determined only by unknown coefficients of , and the near-maximal flavor mixing is not guaranteed in the case of both large angle rotations. These defects disappear by introducing additional discrete symmetries . The quark-lepton mass matrices are presented by taking account of the recent data of atmospheric neutrinos and solar neutrinos.
19 pages, LaTex file, no figures
Cited by in corpus (12)
- Neutrino Masses and Mixing: Evidence and Implications
- Neutrino Masses and Lepton-Flavor Violation in Supersymmetric Models with lopsided Froggatt-Nielsen charges
- Predictive Grand Unified Textures for Quark and Neutrino Masses and Mixings
- Large Mixing Angle MSW Solution in S_3 Flavor Symmetry
- Anomaly-Free Flavor Symmetry and Neutrino Anarchy
- Discrete Flavor Symmetries and Mass Matrix Textures
- Permutation Symmetry for Neutrino and Charged-Lepton Mass Matrices
- Abelian family symmetries and Leptogenesis
- Bilarge Neutrino Mixing and Abelian Flavor Symmetry
- Large Mixing Angle MSW Solution in U(1) Flavor Symmetry
- Quark and Lepton Masses from a {\boldmath } Flavor Symmetry
- Discrete symmetries and neutrino masses