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Impact of the recent results by the CMS and ATLAS collaborations at the CERN Large Hadron Collider on an effective minimal supersymmetric extension of the standard model

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dc.contributor.authorScopel, S.-
dc.contributor.authorChoi, Suyong-
dc.contributor.authorFornengo, N.-
dc.contributor.authorBottino, A.-
dc.date.accessioned2021-09-07T12:20:32Z-
dc.date.available2021-09-07T12:20:32Z-
dc.date.created2021-06-14-
dc.date.issued2011-05-23-
dc.identifier.issn1550-7998-
dc.identifier.urihttps://scholar.korea.ac.kr/handle/2021.sw.korea/112435-
dc.description.abstractWe discuss the impact for light neutralinos in an effective minimal supersymmetric extension of the standard model of the recent results presented by the CMS and ATLAS Collaborations at the CERN Large Hadron Collider for a search of supersymmetry in proton-proton collisions at a center-of-mass energy of 7 TeV with an integrated luminosity of 35 pb(-1). We find that, in the specific case of light neutralinos, efficiencies for the specific signature searched by ATLAS (jets + missing transverse energy and an isolated lepton) imply a lower sensitivity compared to CMS (which searches for jets+ missing transverse energy). Focusing on the CMS bound, if squark soft masses of the three families are assumed to be degenerate, the combination of the ensuing constraint on squark and gluino masses with the experimental limit on the b -> s + gamma decay imply a lower bound on the neutralino mass m(chi) that can reach the value of 11.9 GeV, depending on the gluino mass. On the other hand, when the universality condition among squark soft parameters is relaxed, the lower bound on m(chi) is not constrained by the CMS measurement and then remains at the value 7.5 GeV derived in previous papers.-
dc.languageEnglish-
dc.language.isoen-
dc.publisherAMER PHYSICAL SOC-
dc.titleImpact of the recent results by the CMS and ATLAS collaborations at the CERN Large Hadron Collider on an effective minimal supersymmetric extension of the standard model-
dc.typeArticle-
dc.contributor.affiliatedAuthorChoi, Suyong-
dc.identifier.doi10.1103/PhysRevD.83.095016-
dc.identifier.scopusid2-s2.0-79960774494-
dc.identifier.wosid000290876800004-
dc.identifier.bibliographicCitationPHYSICAL REVIEW D, v.83, no.9-
dc.relation.isPartOfPHYSICAL REVIEW D-
dc.citation.titlePHYSICAL REVIEW D-
dc.citation.volume83-
dc.citation.number9-
dc.type.rimsART-
dc.type.docTypeArticle-
dc.description.journalClass1-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaAstronomy & Astrophysics-
dc.relation.journalResearchAreaPhysics-
dc.relation.journalWebOfScienceCategoryAstronomy & Astrophysics-
dc.relation.journalWebOfScienceCategoryPhysics, Particles & Fields-
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