Neutrino dark matter candidate in fourth generation scenarios

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dc.contributor.authorLee, Hye-Sungko
dc.contributor.authorLiu, Zuoweiko
dc.contributor.authorSoni, Amarjitko
dc.date.accessioned2017-10-23T02:02:08Z-
dc.date.available2017-10-23T02:02:08Z-
dc.date.created2017-10-11-
dc.date.created2017-10-11-
dc.date.created2017-10-11-
dc.date.issued2011-10-
dc.identifier.citationPHYSICS LETTERS B, v.704, no.1-2, pp.30 - 35-
dc.identifier.issn0370-2693-
dc.identifier.urihttp://hdl.handle.net/10203/226493-
dc.description.abstractWe overview the constraints on the 4th-generation neutrino dark matter candidate and investigate a possible way to make it a viable dark matter candidate. Given the LEP constraints tell us that the 4th-generation neutrino has to be rather heavy (> M-Z/2), in sharp contrast to the other three neutrinos, the underlying nature of the 4th-generation neutrino is expected to be different. We suggest that an additional gauge symmetry B - 4L(4) distinguishes it from the standard model's three lighter neutrinos and this also facilitates promotion of the 4th-generation predominantly right-handed neutrino to a good cold dark matter candidate. It provides distinguishable predictions for the dark matter direct detection and the Large Hadron Collider experiments. (C) 2011 Elsevier B.V. All rights reserved.-
dc.languageEnglish-
dc.publisherELSEVIER SCIENCE BV-
dc.titleNeutrino dark matter candidate in fourth generation scenarios-
dc.typeArticle-
dc.identifier.wosid000295750500006-
dc.identifier.scopusid2-s2.0-80052966866-
dc.type.rimsART-
dc.citation.volume704-
dc.citation.issue1-2-
dc.citation.beginningpage30-
dc.citation.endingpage35-
dc.citation.publicationnamePHYSICS LETTERS B-
dc.identifier.doi10.1016/j.physletb.2011.08.051-
dc.contributor.localauthorLee, Hye-Sung-
dc.contributor.nonIdAuthorLiu, Zuowei-
dc.contributor.nonIdAuthorSoni, Amarjit-
dc.description.isOpenAccessN-
dc.type.journalArticleArticle-
dc.subject.keywordPlusELECTROWEAK SYMMETRY-BREAKING-
dc.subject.keywordPlusCP VIOLATION-
dc.subject.keywordPlusGAUGED B-3L(TAU)-
dc.subject.keywordPlusMODEL-
dc.subject.keywordPlusQUARKS-
dc.subject.keywordPlusPHYSICS-
dc.subject.keywordPlusMASSES-
dc.subject.keywordPlusFAMILY-
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