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PhysRevD.88.032002.pdf7.86 MBAdobe PDF見る/開く
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dc.contributor.authorBronner, C.en
dc.contributor.authorHiraki, T.en
dc.contributor.authorHirota, S.en
dc.contributor.authorHuang, K.en
dc.contributor.authorIchikawa, A. K.en
dc.contributor.authorIeki, K.en
dc.contributor.authorIkeda, M.en
dc.contributor.authorKikawa, T.en
dc.contributor.authorKubo, H.en
dc.contributor.authorLitchfield, R. P.en
dc.contributor.authorMinamino, A.en
dc.contributor.authorMurakami, A.en
dc.contributor.authorNagasaki, T.en
dc.contributor.authorNakaya, T.en
dc.contributor.authorOtani, M.en
dc.contributor.authorSuzuki, K.en
dc.contributor.authorTakahashi, S.en
dc.contributor.authorT2K Collaborationen
dc.contributor.alternative市川, 温子ja
dc.contributor.alternative木河, 達也ja
dc.contributor.alternative中家, 剛ja
dc.date.accessioned2020-05-11T08:29:27Z-
dc.date.available2020-05-11T08:29:27Z-
dc.date.issued2013-08-01-
dc.identifier.issn1550-7998-
dc.identifier.urihttp://hdl.handle.net/2433/250791-
dc.description.abstractThe T2K Collaboration reports evidence for electron neutrino appearance at the atmospheric mass splitting, |Δm232|≈2.4×10−3  eV2. An excess of electron neutrino interactions over background is observed from a muon neutrino beam with a peak energy of 0.6 GeV at the Super-Kamiokande (SK) detector 295 km from the beam’s origin. Signal and background predictions are constrained by data from near detectors located 280 m from the neutrino production target. We observe 11 electron neutrino candidate events at the SK detector when a background of 3.3±0.4(syst) events is expected. The background-only hypothesis is rejected with a p value of 0.0009 (3.1σ), and a fit assuming νμ→νe oscillations with sin22θ23=1, δCP=0 and |Δm232|=2.4×10−3  eV2 yields sin22θ13=0.088+0.049−0.039(stat+syst).en
dc.format.mimetypeapplication/pdf-
dc.language.isoeng-
dc.publisherAmerican Physical Society (APS)en
dc.rights© 2013 American Physical Societyen
dc.titleEvidence of electron neutrino appearance in a muon neutrino beamen
dc.typejournal article-
dc.type.niitypeJournal Article-
dc.identifier.jtitlePhysical Review Den
dc.identifier.volume88-
dc.identifier.issue3-
dc.relation.doi10.1103/PhysRevD.88.032002-
dc.textversionpublisher-
dc.identifier.artnum032002-
dcterms.accessRightsopen access-
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