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Phys. Rev. Lett. 93, 101801 (2004) [6 pages]

Evidence for an Oscillatory Signature in Atmospheric Neutrino Oscillations

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Y. Ashie et al. The Super-Kamiokande Collaboration
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Received 27 April 2004; published 3 September 2004

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; 1.9×10-3<Δm2<3.0×10-3  eV2 and sin⁡22θ>0.90 at 90% confidence level.

© 2004 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.93.101801
DOI:
10.1103/PhysRevLett.93.101801
PACS:
14.60.Pq, 96.40.Tv