Tests of neutrino stability
Abstract
A possible solution of the solar neutrino problem is that electron neutrinos decay in transit from the sun. The phenomenological consequences of this hypothesis for solar neutrino experiments with detectors of 2H, 40Ar, 71Ga, 98Mo, and electron-neutrino scattering are discussed. The postulated fast decay can occur in models of majoron type without violating laboratory, cosmological, or astrophysical constraints.
Address after January 1st, 1987: Department de Física Teòrica, Universitat de Valencia, Burjassot, Valencia, Spain.- Publication:
-
Physics Letters B
- Pub Date:
- December 1986
- DOI:
- 10.1016/0370-2693(86)90065-1
- Bibcode:
- 1986PhLB..181..369B