Supersymmetric majoron signatures and solar neutrino oscillations

Publisher Website
Google Scholar
Abstract
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 μ and τ decay spectra for parameter values that substantially reduce the solar neutrino flux. A signature of the model is the possible observation of the decay μ→e+majoron.

This publication has 44 references indexed in Scilit: