Solar Neutrinos with Super-Kamiokande

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dc.creatorSmy, Michael B
dc.date1999-03-16
dc.date.accessioned2026-07-07T03:37:48Z
dc.date.available2026-07-07T03:37:48Z
dc.descriptionThe 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.
dc.description7 pages, 6 figures, LaTeX 2, RevTeX. 11 EPS files included using epsf style. This is part of the proceedings for the DPF'99 Conference
dc.identifierhttps://arxiv.org/abs/hep-ex/9903034
dc.identifierhttp://arxiv.org/abs/hep-ex/9903034
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/38267
dc.subjectHigh Energy Physics - Experiment
dc.titleSolar Neutrinos with Super-Kamiokande
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