Search for Weakly Interacting Massive Particles with the First Five-Tower Data from the Cryogenic Dark Matter Search at the Soudan Underground Laboratory

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dc.contributor.authorAhmed, Zko
dc.contributor.authorAkerib, D. Sko
dc.contributor.authorArrenberg, Sko
dc.contributor.authorAttisha, M. Jko
dc.contributor.authorYoo, Jongheeko
dc.date.accessioned2016-07-25T09:43:42Z-
dc.date.available2016-07-25T09:43:42Z-
dc.date.created2016-07-21-
dc.date.created2016-07-21-
dc.date.created2016-07-21-
dc.date.issued2009-01-
dc.identifier.citationPHYSICAL REVIEW LETTERS, v.102, no.1-
dc.identifier.issn0031-9007-
dc.identifier.urihttp://hdl.handle.net/10203/212197-
dc.description.abstractWe report results from the Cryogenic Dark Matter Search at the Soudan Underground Laboratory (CDMS II) featuring the full complement of 30 detectors. A blind analysis of data taken between October 2006 and July 2007 sets an upper limit on the weakly interacting massive particle (WIMP) nucleon spin-independent cross section of 6.6 x 10(-44) cm(2) (4.6 x 10(-44) cm(2) when combined with previous CDMS II data) at the 90% confidence level for a WIMP mass of 60 GeV/c(2). This achieves the best sensitivity for dark matter WIMPs with masses above 44 GeV/c(2), and significantly restricts the parameter space for some favored supersymmetric models.-
dc.languageEnglish-
dc.publisherAMER PHYSICAL SOC-
dc.titleSearch for Weakly Interacting Massive Particles with the First Five-Tower Data from the Cryogenic Dark Matter Search at the Soudan Underground Laboratory-
dc.typeArticle-
dc.identifier.wosid000262355000008-
dc.identifier.scopusid2-s2.0-58649118638-
dc.type.rimsART-
dc.citation.volume102-
dc.citation.issue1-
dc.citation.publicationnamePHYSICAL REVIEW LETTERS-
dc.identifier.doi10.1103/PhysRevLett.102.011301-
dc.contributor.localauthorYoo, Jonghee-
dc.contributor.nonIdAuthorAhmed, Z-
dc.contributor.nonIdAuthorAkerib, D. S-
dc.contributor.nonIdAuthorArrenberg, S-
dc.contributor.nonIdAuthorAttisha, M. J-
dc.type.journalArticleArticle-
dc.subject.keywordPlusCOSMOLOGICAL CONSTRAINTS-
dc.subject.keywordPlusDAMA/LIBRA-
dc.subject.keywordPlusCANDIDATES-
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