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A Unique Oscillation Solution to the Solar Neutrino Problem?

By M B Smy

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

Topics: Particle Physics - Experiment
Year: 2002
DOI identifier: 10.1142/9789812776488_0006
OAI identifier: oai:cds.cern.ch:537778
Provided by: CERN Document Server

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