Evidence for an Oscillatory Signature in Atmospheric Neutrino Oscillations

Y. Ashie et al. (The Super-Kamiokande Collaboration)
Phys. Rev. Lett. 93, 101801 – Published 3 September 2004

Abstract

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 νμντ neutrino oscillation parameters; 1.9×103<Δm2<3.0×103eV2 and sin22θ>0.90 at 90% confidence level.

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  • Received 27 April 2004

DOI:https://doi.org/10.1103/PhysRevLett.93.101801

©2004 American Physical Society

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Vol. 93, Iss. 10 — 3 September 2004

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