6533b861fe1ef96bd12c5874
RESEARCH PRODUCT
Supersymmetric majoron signatures and solar neutrino oscillations
Jose W.f. ValleArcadi Santamariasubject
PhysicsParticle physicsMuonSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyGeneral Physics and AstronomySolar neutrino problemPartícules (Física nuclear)Nuclear physicsParticle decayHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationLeptonMajorondescription
Spontaneous R-parity breaking in supergravity solves the solar neutrino problem through matter-enhanced neutrino oscillations. The model may be tested in collider experiments and through ``dynamical'' effects associated with the existence of a weakly interacting majoron. Apart from astrophysical effects, majoron emission can produce observable changes in \ensuremath{\mu} and \ensuremath{\tau} decay spectra for parameter values that substantially reduce the solar neutrino flux. A signature of the model is the possible observation of the decay \ensuremath{\mu}\ensuremath{\rightarrow}e+majoron.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 1988-02-01 |