and maximal mixing of
- 29 June 1999
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 60 (3) , 033005
- https://doi.org/10.1103/physrevd.60.033005
Abstract
A flavor symmetry can successfully describe charged fermion masses and mixings, and suppress SUSY FCNC processes, making it a viable candidate for a theory of flavor. We show that a direct application of this flavor symmetry automatically predicts a mixing of 45° for where is a light, right-handed state. The introduction of an additional flavor symmetry acting on the right-handed neutrinos makes the model phenomenologically viable, explaining the solar neutrino deficit as well as the atmospheric neutrino anomaly, while giving a potential hot dark matter candidate and retaining the theory’s predictivity in the quark sector.
Keywords
All Related Versions
This publication has 20 references indexed in Scilit:
- Rescuing grand unification scenario for neutrino massPhysics Letters B, 1998
- Where do we stand with solar neutrino oscillations?Physical Review D, 1998
- Study of the atmospheric neutrino flux in the multi-GeV energy rangePhysics Letters B, 1998
- Results onNeutrino Oscillations from the LSND ExperimentPhysical Review Letters, 1998
- Evidence for Oscillation of Atmospheric NeutrinosPhysical Review Letters, 1998
- CP violation in B decays and supersymmetryNuclear Physics B, 1997
- Neutrino physics from a U(2) flavor symmetryPhysical Review D, 1997
- Consequences of a U(2) flavour symmetryPhysics Letters B, 1997
- Predictions from a U(2) flavour symmetry in supersymmetric theoriesPhysics Letters B, 1996
- Horizontal symmetries for the supersymmetric flavor problemNuclear Physics B, 1996