Evidence for an oscillatory signature in atmospheric neutrino oscillation

By The Super-Kamiokande Collaboration Y.Ashie, et al. 2004

168 citations recorded by the source corpus.

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

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/205c0ead73ef171e5ca34038eec1a32ae779f12a

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In Nuclear and High Energy Physics

1. S. Antusch
2. Y. Farzan
3. M. Tórtola
4. M. Schmidt
5. M. Ratz
6. J. Kersten
7. Manfred Lindner
8. Z. Xing

Citations in the corpus

• Running neutrino mass parameters in see-saw scenarios (2005, background): ““Current” is the current limit from SuperKamiokande [58], “Beams” means conventional neutrino beams.”
• Neutrino oscillations (2013, unknown): “Figure 6: Plot of the number of events versus L/E (L is the distance between the neutrino production and the detector and E is the neutrino energy) for the Super-Kamiokande data (points with error bars); the histogram is the result of the Monte Carlo simulation for atmospheric neutrino events withou”
• Neutrino Oscillations and Non-standard Interactions (2017, background): “Some years later, the Super-Kamiokande Collaboration reported a L/E distribution of the atmospheric νμ data sample characteristic of neutrino oscillations [79].”