Abstract
Muon neutrino disappearance probability as a function of neutrino flight length over neutrino energy was studied. A dip in the distribution was observed in the data, as predicted from the sinusoidal flavor transition probability of neutrino oscillation. The observed distribution constrained neutrino oscillation parameters; and at 90% confidence level.
- Received 27 April 2004
DOI:https://doi.org/10.1103/PhysRevLett.93.101801
©2004 American Physical Society