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Implications for Solar Neutrino Oscillations from Super-Kamiokande and SNO Data

2001/08/31 by Michael B. Smy, Smy, Michael B.
Physics and Astronomy · #FOS: Physical sciences #High Energy Physics - Experiment (hep-ex) #hep-ex

paper · pdf · doi:10.48550/arxiv.hep-ex/0108053

8 pages, 6 figures; to be published in the proceedings of the NO-VE Workshop held in Venice, July 24-26, 2001

arxiv created 2001/08/31 · arxiv updated 2009/11/30

Abstract

Super-Kamiokande uses neutrino-electron elastic scattering to measure the recoil electron spectrum and zenith-angle dependence of solar 8B neutrinos. SNO has measured the 8B neutrino--deuteron charged-current reaction rate. The elastic scattering rate, spectrum and zenith-angle dependence in conjunction with the charged-current reaction rate favors active neutrino oscillations at large mixing angles by about 3σ over the no-oscillation hypothesis and small mixing angles. The analysis is independent of the absolute 8B and \it hep flux and assumes two-flavor oscillations described by mixing angle and mass2 difference. Two allowed regions at large mixing are found.

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