Solar Neutrino Precision Measurements using all 1496 Days of Super-Kamiokande-I Data
arXiv:hep-ex/0208004 · doi:10.1016/S0920-5632(03)01300-8
Abstract
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.
to be published in the Proceedings of the XXth International Confernece on Neutrino Physics and Astrophysics 8 pages, 11 figures