Solar-neutrino-oscillation parameters and the broken-R-parity Majoron

Details Solar-neutrino-oscillation parameters and the broken-R-parity Majoron Solar-neutrino-oscillation parameters and the broken-R-parity Majoron

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvd..39.1780s&link_type=abstract

Physical Review D (Particles and Fields), Volume 39, Issue 6, 15 March 1989, pp.1780-1783

Other

65

Charge Conjugation, Parity, Time Reversal, And Other Discrete Symmetries

Scientific paper

Matter-enhanced neutrino-oscillation parameters can be probed in a variety of conventional experiments in supergravity models where the small neutrino mass arises from spontaneous R-parity violation. A combined analysis of astrophysical and laboratory limits tends to exclude regions of oscillation parameters where the high-energy neutrinos are adiabatically converted. This suggests the possibility of a large reduction in the pp and 7Be neutrino flux even for a mildly reduced 8B neutrino flux, thus stressing the importance of gallium experiments.

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