A simple modification of the maximal mixing scenario for three light neutrinos

Cited 26 time in webofscience Cited 0 time in scopus
  • Hit : 370
  • Download : 0
DC FieldValueLanguage
dc.contributor.authorKang, KSko
dc.contributor.authorKim, JEko
dc.contributor.authorKo, Pyungwonko
dc.date.accessioned2013-02-28T06:50:06Z-
dc.date.available2013-02-28T06:50:06Z-
dc.date.created2012-02-06-
dc.date.created2012-02-06-
dc.date.issued1996-11-
dc.identifier.citationZEITSCHRIFT FUR PHYSIK C-PARTICLES AND FIELDS, v.72, no.4, pp.671 - 675-
dc.identifier.issn0170-9739-
dc.identifier.urihttp://hdl.handle.net/10203/73337-
dc.description.abstractWe suggest a simple modification of the maximal mixing scenario (with Sg permutation symmetry) for three light neutrinos. Our neutrino mass matrix has smaller permutation symmetry S-2(nu(mu) reversible arrow nu(e)), and is consistent with all neutrino experiments except the Cl-37 experiment. The resulting mass eigenvalues for three neutrinos are m(1) approximate to (2.55 - 1.27) x 10(-3) eV, m(2,3) approximate to (0.71 - 1.43) eV for Delta m(LSND)(2) = 0.5 - 2.0 eV(2). Then these light neutrinos can account for similar to (2.4 - 4.8)% (6.2 - 12.4%) of the dark matter for h = 0.8 (0.5). Our model predicts the nu(mu) --> nu(tau) oscillation probability in the range sensitive to the future experiments such as CHORUS and NOMAD.-
dc.languageEnglish-
dc.publisherSPRINGER-
dc.subjectKAMIOKANDE-II DETECTOR-
dc.subjectSOLAR NEUTRINOS-
dc.subjectCROSS-SECTION-
dc.subjectPOWER-REACTOR-
dc.subjectREAL-TIME-
dc.subjectSEARCH-
dc.subjectOSCILLATIONS-
dc.subjectGALLEX-
dc.subjectFLUX-
dc.subject(NU)OVER-BAR(MU)-&gt-
dc.subject(NU)OVER-BAR(E)-
dc.titleA simple modification of the maximal mixing scenario for three light neutrinos-
dc.typeArticle-
dc.identifier.wosidA1996VW68800016-
dc.type.rimsART-
dc.citation.volume72-
dc.citation.issue4-
dc.citation.beginningpage671-
dc.citation.endingpage675-
dc.citation.publicationnameZEITSCHRIFT FUR PHYSIK C-PARTICLES AND FIELDS-
dc.identifier.doi10.1007/s002880050291-
dc.contributor.nonIdAuthorKang, KS-
dc.contributor.nonIdAuthorKim, JE-
dc.type.journalArticleArticle-
dc.subject.keywordPlusKAMIOKANDE-II DETECTOR-
dc.subject.keywordPlusSOLAR NEUTRINOS-
dc.subject.keywordPlusCROSS-SECTION-
dc.subject.keywordPlusPOWER-REACTOR-
dc.subject.keywordPlusREAL-TIME-
dc.subject.keywordPlusSEARCH-
dc.subject.keywordPlusOSCILLATIONS-
dc.subject.keywordPlusGALLEX-
dc.subject.keywordPlusFLUX-
dc.subject.keywordPlus(NU)OVER-BAR(MU)-&gt-
dc.subject.keywordPlus(NU)OVER-BAR(E)-
Appears in Collection
Files in This Item
There are no files associated with this item.
This item is cited by other documents in WoS
⊙ Detail Information in WoSⓡ Click to see webofscience_button
⊙ Cited 26 items in WoS Click to see citing articles in records_button

qr_code

  • mendeley

    citeulike


rss_1.0 rss_2.0 atom_1.0