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Solar Neutrinos with Super-Kamiokande

Michael B Smy
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Abstract

The discrepancy of the measured solar neutrino flux compared to the predictions of the standard solar model may be explained by the neutrino flavor oscillation hypothesis. A more direct and less model-dependent test of this hypothesis is a measurement of the distortion of the shape of the solar neutrino energy spectrum. Super-Kamiokande studies the energy spectrum of recoil electrons from solar neutrino scattering in water above 5.5 MeV.

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Michael B Smy. 1999-03-16. Solar Neutrinos with Super-Kamiokande. https://arxiv.org/abs/hep-ex/9903034

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