A Unique Oscillation Solution to the Solar Neutrino Problem?
arXiv:hep-ex/0202020 · doi:10.1142/9789812776488_0006
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 mass^2 difference between the two mass eigenstates is Delta m^2 approx 3-25 x 10^-5 eV^2, the mixing angle theta is tan^2 theta approx 0.21-0.67.
10 pages, 3 figures, to be published in the proceedings of the NOON 2001 workshop