Measurement of the flux and zenith-angle distribution of upward through-going muons by Super-Kamiokande

dc.creatorKamiokande Collaboration
dc.date1998-12-11
dc.date1999-03-18
dc.date.accessioned2026-07-07T10:32:21Z
dc.date.available2026-07-07T10:32:21Z
dc.descriptionA total of 614 upward through-going muons of minimum energy 1.6 GeV are observed by Super-Kamiokande during 537 detector live days. The measured muon flux is 1.74+/-0.07(stat.)+/-0.02(sys.)x10^{-13}cm^{-2}s^{-1}sr^{-1} compared to an expected flux of 1.97+/-0.44(theo.)x10^{-13}cm^{-2}s^{-1}sr^{-1}. The absolute measured flux is in agreement with the prediction within the errors. However, the zenith angle dependence of the observed upward through-going muon flux does not agree with no-oscillation predictions. The observed distortion in shape is consistent with the ν_μ<-> ν_τoscillation hypothesis with \sin^22θ> 0.4 and 1x10^{-3} < Δm^2 < 1x10^{-1} eV^{2} at 90% confidence level.
dc.description8 pages w/ 3 figures new version contains minor fixes, as it appears in PRL
dc.identifierhttps://arxiv.org/abs/hep-ex/9812014
dc.identifierhttp://arxiv.org/abs/hep-ex/9812014
dc.identifierPhys.Rev.Lett.82:2644-2648,1999
dc.identifierdoi:10.1103/PhysRevLett.82.2644
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178725
dc.subjectHigh Energy Physics - Experiment
dc.titleMeasurement of the flux and zenith-angle distribution of upward through-going muons by Super-Kamiokande
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