SO(3) gauge model for neutrino masses and oscillations
Creators
Description
I mainly describe neutrino masses and oscillations in the gauge model with SO(3)F lepton flavor symmetry and with two Higgs triplets. It is shown how the maximal mixing between νμ and ντ neutrinos comes out naturally after spontaneous breaking of the symmetry. The nearly two-flavor mixing scenario is resulted naturally from an approximate permutation symmetry between the two Higgs triplets. The hierarchy between the neutrino mass- squared differences, which is needed for reconciling both solar and atmospheric neutrino data, leads to an almost maximal mixing between νe and νμ neutrinos. Thus the model favors the intriguing bi-maximal mixing scenario. The three Majorana neutrino masses are allowed to be nearly degenerate and large enough to play a significant cosmological role. The model can also lead to interesting phenomena on lepton-flavor violations via the SO(3)F gauge interactions
Additional details
Identifiers
- PII
- S0920563200005065;
Publishing Information
- Journal Title
- Nuclear Physics. B, Proceedings Supplements
- Journal Volume
- 85
- Journal Issue
- 1-3
- Journal Page Range
- p. 193-198
- ISSN
- 0920-5632
- CODEN
- NPBSE7
Conference
- Title
- 6. topical seminar on neutrino and astroparticle physics
- Dates
- 17-21 May 1999
- Place
- Pisa (Italy)
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 34062255
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- FLAVOR MODEL; MAJORANA THEORY; MASS; NEUTRINO OSCILLATION; SO-3 GROUPS; SOLAR NEUTRINOS; UNIFIED GAUGE MODELS
- Descriptors DEC
- COMPOSITE MODELS; ELEMENTARY PARTICLES; FERMIONS; FIELD THEORIES; LEPTONS; LIE GROUPS; MASSLESS PARTICLES; MATHEMATICAL MODELS; NEUTRINOS; PARTICLE MODELS; QUANTUM FIELD THEORY; QUARK MODEL; RADIATIONS; SO GROUPS; SOLAR PARTICLES; SOLAR RADIATION; STELLAR RADIATION; SYMMETRY GROUPS
Optional Information
- Copyright
- Copyright (c) 2000 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.