THE MSW EFFECT FOR MAJORANA NEUTRINO

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dc.contributor.authorLEE, JSko
dc.contributor.authorKWON, HMko
dc.contributor.authorKim, Jae Kwanko
dc.date.accessioned2013-02-27T12:26:35Z-
dc.date.available2013-02-27T12:26:35Z-
dc.date.created2012-02-06-
dc.date.created2012-02-06-
dc.date.issued1995-07-
dc.identifier.citationMODERN PHYSICS LETTERS A, v.10, no.22, pp.1593 - 1599-
dc.identifier.issn0217-7323-
dc.identifier.urihttp://hdl.handle.net/10203/68575-
dc.description.abstractWe study the MSW effect when neutrinos are the Majorana particles with a nonvanishing CP-violating phase using the method based on the neutrino energy eigenstates in a medium with varying density. We calculate the transition probability P(nu(e) --> nu(e)) as a function of the ratio of neutrino energy to neutrino mass difference E/Delta(0) in the solar neutrino case for several values of the mixing angle theta and the CP-violating phase sigma. We observe that the overall shape of the transition probability is not affected by the phase sigma.-
dc.languageEnglish-
dc.publisherWORLD SCIENTIFIC PUBL CO PTE LTD-
dc.subjectOSCILLATIONS-
dc.subjectMATTER-
dc.subjectHELIOSEISMOLOGY-
dc.subjectSPECTROSCOPY-
dc.subjectENHANCEMENT-
dc.subjectSEARCH-
dc.subjectMODEL-
dc.subjectFLUX-
dc.subjectSUN-
dc.titleTHE MSW EFFECT FOR MAJORANA NEUTRINO-
dc.typeArticle-
dc.identifier.wosidA1995RP59900003-
dc.type.rimsART-
dc.citation.volume10-
dc.citation.issue22-
dc.citation.beginningpage1593-
dc.citation.endingpage1599-
dc.citation.publicationnameMODERN PHYSICS LETTERS A-
dc.identifier.doi10.1142/S021773239500171X-
dc.contributor.nonIdAuthorLEE, JS-
dc.contributor.nonIdAuthorKWON, HM-
dc.type.journalArticleArticle-
dc.subject.keywordPlusOSCILLATIONS-
dc.subject.keywordPlusMATTER-
dc.subject.keywordPlusHELIOSEISMOLOGY-
dc.subject.keywordPlusSPECTROSCOPY-
dc.subject.keywordPlusENHANCEMENT-
dc.subject.keywordPlusSEARCH-
dc.subject.keywordPlusMODEL-
dc.subject.keywordPlusFLUX-
dc.subject.keywordPlusSUN-
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