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Search for dark matter and unparticles produced in association with a Z boson in proton-proton collisions at root s=8 TeV

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dc.contributor.authorKhachatryan, V.-
dc.contributor.authorSirunyan, A. M.-
dc.contributor.authorTumasyan, A .-
dc.contributor.authorAdam, W.-
dc.contributor.authorAsilar, E.-
dc.contributor.authorBergauer, T.-
dc.contributor.authorBrandstetter, J.-
dc.contributor.authorBrondolin, E.-
dc.contributor.authorDragicevic, M.-
dc.contributor.authorKim, Tae Jeong-
dc.date.accessioned2022-07-15T18:03:16Z-
dc.date.available2022-07-15T18:03:16Z-
dc.date.created2021-05-14-
dc.date.issued2016-03-
dc.identifier.issn2470-0010-
dc.identifier.urihttps://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/154906-
dc.description.abstractA search for evidence of particle dark matter (DM) and unparticle production at the LHC has been performed using events containing two charged leptons, consistent with the decay of a Z boson, and large missing transverse momentum. This study is based on data collected with the CMS detector corresponding to an integrated luminosity of 19.7 fb(-1) of pp collisions at the LHC at a center-of-mass energy of 8 TeV. No significant excess of events is observed above the number expected from the standard model contributions. The results are interpreted in terms of 90% confidence level limits on the DM-nucleon scattering cross section, as a function of the DM particle mass, for both spin-dependent and spin-independent scenarios. Limits are set on the effective cutoff scale., and on the annihilation rate for DM particles, assuming that their branching fraction to quarks is 100%. Additionally, the most stringent 95% confidence level limits to date on the unparticle model parameters are obtained.-
dc.language영어-
dc.language.isoen-
dc.publisherAMER PHYSICAL SOC-
dc.titleSearch for dark matter and unparticles produced in association with a Z boson in proton-proton collisions at root s=8 TeV-
dc.typeArticle-
dc.contributor.affiliatedAuthorKim, Tae Jeong-
dc.identifier.doi10.1103/PhysRevD.93.052011-
dc.identifier.scopusid2-s2.0-84963973501-
dc.identifier.wosid000372720400001-
dc.identifier.bibliographicCitationPHYSICAL REVIEW D, v.93, pp.1 - 29-
dc.relation.isPartOfPHYSICAL REVIEW D-
dc.citation.titlePHYSICAL REVIEW D-
dc.citation.volume93-
dc.citation.startPage1-
dc.citation.endPage29-
dc.type.rimsART-
dc.type.docType정기학술지(Article(Perspective Article포함))-
dc.description.journalClass1-
dc.description.isOpenAccessY-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaAstronomy & Astrophysics-
dc.relation.journalResearchAreaPhysics-
dc.relation.journalWebOfScienceCategoryAstronomy & Astrophysics-
dc.relation.journalWebOfScienceCategoryPhysics, Particles & Fields-
dc.subject.keywordPlusPARTON DISTRIBUTIONS-
dc.subject.keywordPlusCOMPUTATION-
dc.subject.keywordPlusSIMULATION-
dc.subject.keywordPlusEXISTENCE-
dc.subject.keywordPlusMODEL-
dc.identifier.urlhttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.93.052011-
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