Oscillation Solutions to Solar Neutrino Problem

Details Oscillation Solutions to Solar Neutrino Problem Oscillation Solutions to Solar Neutrino Problem

1999-04-07

arxiv.org/abs/hep-ph/9904259v2

Nucl.Phys.Proc.Suppl.80:17-32,2000

Physics

High Energy Physics

High Energy Physics - Phenomenology

Plenary talk at 19th texas Symposium. New references added

Scientific paper

10.1016/S0920-5632(99)00826-9

The current status of oscillation solutions to the Solar Neutrino Problem is reviewed. Four oscillation solutions are discussed in the light of 708d Superkamiokande data: MSW, Just-So VO, VO with Energy-Independent Suppression (EIS) and Resonant-Spin-Flavor-Precession (RSFP). Only EIS VO is strongly disfavoured by the global rates, mostly due to the Homestake data. Vacuum oscillations give an interesting solution which explains high-energy excess of events observed by Superkamiokande and predicts {\em semi-annual} seasonal variation of $Be$-neutrino flux. There are indications to these variations in the GALLEX and Homestake data. No direct evidence for oscillation is found yet.

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