DC Field | Value | Language |
---|---|---|
dc.contributor.author | Abe, K | ko |
dc.contributor.author | Hayato, Y | ko |
dc.contributor.author | Iida, T | ko |
dc.contributor.author | Ishihara, K | ko |
dc.contributor.author | Yoo, Jonghee | ko |
dc.date.accessioned | 2016-09-06T07:25:16Z | - |
dc.date.available | 2016-09-06T07:25:16Z | - |
dc.date.created | 2016-07-22 | - |
dc.date.created | 2016-07-22 | - |
dc.date.issued | 2006-10 | - |
dc.identifier.citation | PHYSICAL REVIEW LETTERS, v.97, no.17 | - |
dc.identifier.issn | 0031-9007 | - |
dc.identifier.uri | http://hdl.handle.net/10203/212316 | - |
dc.description.abstract | A search for the appearance of tau neutrinos from nu(mu)<->nu(tau) oscillations in the atmospheric neutrinos has been performed using 1489.2 days of atmospheric neutrino data from the Super-Kamiokande-I experiment. A best fit tau neutrino appearance signal of 138 +/- 48(stat)+15/-32(syst) events is obtained with an expectation of 78 +/- 26(syst). The hypothesis of no tau neutrino appearance is disfavored by 2.4 sigma. | - |
dc.language | English | - |
dc.publisher | AMER PHYSICAL SOC | - |
dc.subject | OSCILLATIONS | - |
dc.subject | ANNIHILATION | - |
dc.subject | DETECTOR | - |
dc.title | Measurement of atmospheric neutrino flux consistent with tau neutrino appearance | - |
dc.type | Article | - |
dc.identifier.wosid | 000241586800017 | - |
dc.identifier.scopusid | 2-s2.0-33750292476 | - |
dc.type.rims | ART | - |
dc.citation.volume | 97 | - |
dc.citation.issue | 17 | - |
dc.citation.publicationname | PHYSICAL REVIEW LETTERS | - |
dc.identifier.doi | 10.1103/PhysRevLett.97.171801 | - |
dc.contributor.localauthor | Yoo, Jonghee | - |
dc.contributor.nonIdAuthor | Abe, K | - |
dc.contributor.nonIdAuthor | Hayato, Y | - |
dc.contributor.nonIdAuthor | Iida, T | - |
dc.contributor.nonIdAuthor | Ishihara, K | - |
dc.type.journalArticle | Article | - |
dc.subject.keywordPlus | OSCILLATIONS | - |
dc.subject.keywordPlus | ANNIHILATION | - |
dc.subject.keywordPlus | DETECTOR | - |
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