arXiv · hep-ex/0208004
Solar Neutrino Precision Measurements using all 1496 Days of Super-Kamiokande-I Data
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.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
M. B. Smy. 2002-08-05. Solar Neutrino Precision Measurements using all 1496 Days of Super-Kamiokande-I Data. https://doi.org/10.1016/s0920-5632(03)01300-8
Cite the original work for its findings. Save a collection to share your selection of sources.