Toward the confirmation of atmospheric neutrino oscillations
arXiv:2308.13162 · doi:10.1093/ptep/ptad097
Abstract
The atmospheric muon neutrino deficit, which was possible evidence of oscillation, was reported by the Kamiokande experiment from 1988. Many experimental efforts were made to examine the Kamiokande results. Experiments which contributed to the confirmation of oscillation are reviewed. Especially, long-baseline neutrino-oscillation experiments are described in detail.
arXiv comment15 pages, 11 figures, accepted by Prog. Theor. Exp. Phys. as a paper for "A special issue in memory of Masatoshi Koshiba, a pioneer in experimental particle physics and astrophysics"
References in corpus (11)
- Evidence for oscillation of atmospheric neutrinos
- Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory
- Indication of Electron Neutrino Appearance from an Accelerator-produced Off-axis Muon Neutrino Beam
- Measurements of the Solar Neutrino Flux from Super-Kamiokande's First 300 Days
- Observation of muon neutrino disappearance with the MINOS detectors and the NuMI neutrino beam
- Evidence for muon neutrino oscillation in an accelerator-based experiment
- First measurement of electron neutrino appearance in NOvA
- Physics Potential of a Long Baseline Neutrino Oscillation Experiment Using J-PARC Neutrino Beam and Hyper-Kamiokande
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- The start of things for Kamiokande: The Kamioka Nucleon Decay Experiment