Evidence for an oscillatory signature in atmospheric neutrino oscillation

et al; The Super-Kamiokande Collaboration: Y.Ashie

Evidence for an oscillatory signature in atmospheric neutrino oscillation

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arxiv hep-ex/0404034 v1 pith:B4XZFEGC submitted 2004-04-27 hep-ex

The Super-Kamiokande Collaboration: Y.Ashie , et al This is my paper · ORCID

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keywords neutrinooscillationdistributionobservedprobabilityatmosphericconfidenceconstrained

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Muon neutrino disappearance probability as a function of neutrino flight length L over neutrino energy E was studied. A dip in the L/E distribution was observed in the data, as predicted from the sinusoidal flavor transition probability of neutrino oscillation. The observed L/E distribution constrained nu_mu <-> nu_tau neutrino oscillation parameters; 1.9x10^-3 < Delta m^2 < 3.0x10^-3 eV^2 and \sin^2(2theta) > 0.90 at 90% confidence level.

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