Results from solar-neutrino experiments.

Details Results from solar-neutrino experiments. Results from solar-neutrino experiments.

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ncimc..19..821k&link_type=abstract

Nuovo Cimento C, Vol. 19C, N. 6, p. 821 - 833

Physics

6

Solar Neutrinos: Models, Solar Neutrinos: Detectors

Scientific paper

All four operating solar-neutrino detectors (HOMESTAKE, KAMIOKANDE, GALLEX, SAGE) get positive results but below the level expected from solar models. Taking all data together, it appears that the abundant pp-neutrinos are fully present, the intermediate 7Be-neutrinos are strongly or totally suppressed and the rare 8B-neutrinos are partially reduced (by a factor 2 - 3). This cannot be explained by modifications of the stellar model but would be consistent with neutrino flavour oscillations between the solar core and the detector. If this applies, non-zero neutrino mass is required. The evidence is summarized and discussed.

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