Another Look at Just-So Solar Neutrino Oscillations

Details Another Look at Just-So Solar Neutrino Oscillations Another Look at Just-So Solar Neutrino Oscillations

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...193.7908g&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #79.08; Bulletin of the American Astronomical Society, Vol. 30, p.1373

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Scientific paper

We take another look at ``Just-So'' solar neutrino oscillations and characterize them by the energy at which the distance-varying angle is pi /2. The SuperKamiokande spectrum can be fit with an energy in the range of 9-12 MeV. In this case, the pp neutrinos are reduced to half the standard solar model prediction and (7) Be neutrinos must make up a significant part of the gallium signal, in contrast to the small-angle MSW prediction. Furthermore, the (7) Be neutrinos could show a large seasonal variation, which might be detectable in more precise gallium data.

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