Super Kamiokande results: atmospheric and solar neutrinos

Physics – High Energy Physics – High Energy Physics - Experiment

Scientific paper

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8 pages, 7 figures, Proceedings for the XXXIXth Rencontres de Moriond on Electroweak Interactions (2004)

Scientific paper

Atmospheric neutrino and solar neutrino data from the first phase of Super-Kamiokande (SK-I) are presented. The observed data are used to study atmospheric and solar neutrino oscillations. Zenith angle distributions from various atmospheric neutrino data samples are used to estimate the neutrino oscillation parameter region. In addition, a new result of the $L/E$ measurement is presented. A dip in the $L/E$ distribution was observed in the data, as predicted from the sinusoidal flavor transition probability of neutrino oscillation. The energy spectrum and the time variation such as day/night and seasonal differences of solar neutrino flux are measured in Super-Kamiokande. The neutrino oscillation parameters are strongly constrained from those measurements.

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