Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1995-11-03
Phys.Lett. B368 (1996) 112-118
Physics
High Energy Physics
High Energy Physics - Phenomenology
14 pages, latex, epsf, 5 figures; to appear in Phys Lett B
Scientific paper
10.1016/0370-2693(95)01489-6
Both gravitational and mass induced neutrino oscillation mechanisms provide possible resolutions to the Solar Neutrino Problem. The distinguishing feature between the two mechanisms is their dependence on the neutrino energy. We investigate the implications of this by computing the $\B$ neutrino spectrum as determined from each mechanism using a realistic three--flavor evolution model. We find that in the limit of small $\tetau$ mixing angle, the differences are significant enough to observe in future solar neutrino experiments.
Mann Robert B.
Mureika Jonas Roman
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