Solar Neutrino Precision Measurements using all 1496 Days of Super-Kamiokande-I Data

Physics – High Energy Physics – High Energy Physics - Experiment

Scientific paper

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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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