Mikheyev-Smirnov-Wolfenstein effect with flavor-changing neutrino interactions
- National Aeronautics and Space Administration Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois (USA)
We consider the effect that flavor-nondiagonal neutrino interactions with matter have on the resonant {nu} oscillations. It is shown that, even in the absence of {nu} mixing in a vacuum, an efficient conversion of the electron neutrinos from the Sun to another {nu} flavor can result if the strength of this interaction is {similar to}10{sup {minus}2}{ital G}{sub {ital F}}. We show how this can be implemented in the minimal supersymmetric standard model with {ital R}-parity breaking. Here, the {ital L}-violating couplings induce neutrino masses, mixings, and the flavor-nondiagonal neutrino interactions that can provide a Mikheyev-Smirnov-Wolfenstein-like solution to the solar-neutrino problem even for negligible vacuum mixings.
- OSTI ID:
- 5310369
- Journal Information:
- Physical Review, D (Particles Fields); (United States), Vol. 44:4; ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
NEUTRINO OSCILLATION
NEUTRINO-NUCLEON INTERACTIONS
FLAVOR MODEL
SOLAR NEUTRINOS
EIGENSTATES
ELECTRON NEUTRINOS
INVARIANCE PRINCIPLES
LEPTON NUMBER
MASS
PROBABILITY
STANDARD MODEL
SUPERSYMMETRY
COMPOSITE MODELS
ELEMENTARY PARTICLES
FERMIONS
INTERACTIONS
LEPTON-BARYON INTERACTIONS
LEPTON-HADRON INTERACTIONS
LEPTON-NUCLEON INTERACTIONS
LEPTONS
MASSLESS PARTICLES
MATHEMATICAL MODELS
NEUTRINOS
PARTICLE INTERACTIONS
PARTICLE MODELS
QUARK MODEL
RADIATIONS
SOLAR PARTICLES
SOLAR RADIATION
STELLAR RADIATION
SYMMETRY
UNIFIED GAUGE MODELS
645203* - High Energy Physics- Particle Interactions & Properties-Theoretical- Weak Interactions & Properties
645300 - High Energy Physics- Particle Invariance Principles & Symmetries