DC Field | Value | Language |
---|---|---|
dc.contributor.author | Ashie, Y | ko |
dc.contributor.author | Hosaka, J | ko |
dc.contributor.author | Ishihara, K | ko |
dc.contributor.author | Itow, Y | ko |
dc.contributor.author | Yoo, Jonghee | ko |
dc.date.accessioned | 2016-09-06T07:26:30Z | - |
dc.date.available | 2016-09-06T07:26:30Z | - |
dc.date.created | 2016-07-22 | - |
dc.date.created | 2016-07-22 | - |
dc.date.issued | 2004-09 | - |
dc.identifier.citation | PHYSICAL REVIEW LETTERS, v.93, no.10 | - |
dc.identifier.issn | 0031-9007 | - |
dc.identifier.uri | http://hdl.handle.net/10203/212328 | - |
dc.description.abstract | 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 the sinusoidal flavor transition probability of neutrino oscillation. The observed L/E distribution constrained nu(mu)<---->nu(tau) neutrino oscillation parameters; 1.9x10(-3)<Deltam(2)<3.0x10(-3) eV(2) and sin(2)2theta>0.90 at 90% confidence level. | - |
dc.language | English | - |
dc.publisher | AMER PHYSICAL SOC | - |
dc.subject | ELECTRON-NEUTRINO | - |
dc.subject | FLUX | - |
dc.title | Evidence for an oscillatory signature in atmospheric neutrino oscillations | - |
dc.type | Article | - |
dc.identifier.wosid | 000223717600008 | - |
dc.identifier.scopusid | 2-s2.0-20844449061 | - |
dc.type.rims | ART | - |
dc.citation.volume | 93 | - |
dc.citation.issue | 10 | - |
dc.citation.publicationname | PHYSICAL REVIEW LETTERS | - |
dc.identifier.doi | 10.1103/PhysRevLett.93.101801 | - |
dc.contributor.localauthor | Yoo, Jonghee | - |
dc.contributor.nonIdAuthor | Ashie, Y | - |
dc.contributor.nonIdAuthor | Hosaka, J | - |
dc.contributor.nonIdAuthor | Ishihara, K | - |
dc.contributor.nonIdAuthor | Itow, Y | - |
dc.type.journalArticle | Article | - |
dc.subject.keywordPlus | ELECTRON-NEUTRINO | - |
dc.subject.keywordPlus | FLUX | - |
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