A Unique Oscillation Solution to the Solar Neutrino Problem?
Abstract
A global two-neutrino oscillation fit combining Super-Kamiokande solar neutrino data with the solar neutrino rates measured by Homestake, Gallex/GNO, SAGE and SNO prefers a single allowed area, the Large Mixing Angle solution, at about 95% confidence level. The mass2 difference between the two mass eigenstates is Delta m2 approx 3-25 x 10-5 eV2, the mixing angle theta is tan2 theta approx 0.21-0.67.
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