Revival of the thermal sneutrino dark matter

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dc.contributor.authorLee, Hye-Sungko
dc.contributor.authorMatchev, Konstantin T.ko
dc.contributor.authorNasri, Salahko
dc.date.accessioned2017-10-23T02:02:31Z-
dc.date.available2017-10-23T02:02:31Z-
dc.date.created2017-10-11-
dc.date.created2017-10-11-
dc.date.created2017-10-11-
dc.date.issued2007-08-
dc.identifier.citationPHYSICAL REVIEW D, v.76, no.4-
dc.identifier.issn1550-7998-
dc.identifier.urihttp://hdl.handle.net/10203/226504-
dc.description.abstractThe left-handed sneutrino in the minimal supersymmetric standard model (MSSM) has been ruled out as a viable thermal dark matter candidate, due to conflicting constraints from direct detection experiments and from the measurement of the dark matter relic density. The intrinsic fine-tuning problem of the MSSM, however, motivates an extension with a new U(1)(') gauge symmetry. We show that in the U(1)(')-extended MSSM the right-handed sneutrino nu(R) becomes a good thermal dark matter candidate. We identify two generic parameter space regions where the combined constraints from relic density determinations, direct detection, and collider searches are all satisfied.-
dc.languageEnglish-
dc.publisherAMER PHYSICAL SOC-
dc.titleRevival of the thermal sneutrino dark matter-
dc.typeArticle-
dc.identifier.wosid000249155800002-
dc.identifier.scopusid2-s2.0-34548100267-
dc.type.rimsART-
dc.citation.volume76-
dc.citation.issue4-
dc.citation.publicationnamePHYSICAL REVIEW D-
dc.identifier.doi10.1103/PhysRevD.76.041302-
dc.contributor.localauthorLee, Hye-Sung-
dc.contributor.nonIdAuthorMatchev, Konstantin T.-
dc.contributor.nonIdAuthorNasri, Salah-
dc.description.isOpenAccessN-
dc.type.journalArticleArticle-
dc.subject.keywordPlusSUPERSYMMETRIC STANDARD MODEL-
dc.subject.keywordPlusSCALAR NEUTRINOS-
dc.subject.keywordPlusMU-PROBLEM-
dc.subject.keywordPlusPARTICLES-
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