Physics – High Energy Physics – High Energy Physics - Experiment
Scientific paper
2002-08-05
Nucl.Phys.Proc.Suppl.118:25-32,2003
Physics
High Energy Physics
High Energy Physics - Experiment
to be published in the Proceedings of the XXth International Confernece on Neutrino Physics and Astrophysics 8 pages, 11 figur
Scientific paper
10.1016/S0920-5632(03)01300-8
The results of the entire Super-Kamiokande-I solar neutrino data are presented. The measured interaction rate is 47+-2% of the rate expected by the standard solar model and 133+-5% of the rate implied by the SNO charged-current interaction rate. There is no evidence for spectral distortion or a time dependent neutrino flux. Together with the rates of other experiments, the Super-Kamiokande results imply active solar neutrino oscillations and restrict neutrino mixing and mass square difference to lie within the LMA solution area.
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