Please use this identifier to cite or link to this item: https://hdl.handle.net/11147/8723
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dc.contributor.authorSirunyan, A.M.-
dc.contributor.authorTumasyan, A.-
dc.contributor.authorAdam, W.-
dc.contributor.authorAmbrogi, F.-
dc.contributor.authorAsilar, E.-
dc.contributor.authorBergauer, T.-
dc.contributor.authorGarcia-Ferrero, J.-
dc.date.accessioned2020-07-18T08:28:31Z-
dc.date.available2020-07-18T08:28:31Z-
dc.date.issued2018-
dc.identifier.issn2470-0010-
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.97.032009-
dc.description.abstractA search for new physics is presented in final states with two oppositely charged leptons (electrons or muons), jets identified as originating from b quarks, and missing transverse momentum (pTmiss). The search uses proton-proton collision data at s=13 TeV amounting to 35.9 fb-1 of integrated luminosity collected using the CMS detector in 2016. Hypothetical signal events are efficiently separated from the dominant tt background with requirements on pTmiss and transverse-mass variables. No significant deviation is observed from the expected background. Exclusion limits are set in the context of simplified supersymmetric models with pair-produced top squarks. For top squarks, decaying exclusively to a top quark and a neutralino, exclusion limits are placed at 95% confidence level on the mass of the lightest top squark up to 800 GeV and on the lightest neutralino up to 360 GeV. These results, combined with searches in the single-lepton and all-jet final states, raise the exclusion limits up to 1050 GeV for the lightest top squark and up to 500 GeV for the lightest neutralino. For top squarks undergoing a cascade decay through charginos and sleptons, the mass limits reach up to 1300 GeV for top squarks and up to 800 GeV for the lightest neutralino. The results are also interpreted in a simplified model with a dark matter (DM) particle coupled to the top quark through a scalar or pseudoscalar mediator. For light DM, mediator masses up to 100 (50) GeV are excluded for scalar (pseudoscalar) mediators. The result for the scalar mediator achieves some of the most stringent limits to date in this model. © 2018 CERN.en_US
dc.description.sponsorship; National Science Foundation, NSF, (1151640, 1506130, 1506168, 1508869, 1606321); National Science Foundation, NSF; National Institutes of Health, NIH; U.S. Department of Energy, DOE; Hispanics in Philanthropy, HIP; California Department of Fish and Game, DFG; Qatar National Research Fund, QNRF; Türkiye Atom Enerjisi Kurumu, TAEK; Horizon 2020 Framework Programme, H2020, (675440); Horizon 2020 Framework Programme, H2020; Santa Fe Institute, SFI; Science and Technology Facilities Council, STFC, (GRIDPP, ST/N000242/1); Science and Technology Facilities Council, STFC; European Research Council, ERC; Department of Atomic Energy, Government of India, DAE; Fundação de Amparo à Pesquisa do Estado de São Paulo, FAPESP; National Natural Science Foundation of China, NSFC; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior, CAPES; Chinese Academy of Sciences, CAS; Austrian Science Fund, FWF; Fonds De La Recherche Scientifique - FNRS, FNRS; Chulalongkorn University, CU; Federación Española de Enfermedades Raras, FEDER; Fonds Wetenschappelijk Onderzoek, FWO; Országos Tudományos Kutatási Alapprogramok, OTKA; Conselho Nacional de Desenvolvimento Científico e Tecnológico, CNPq; National Research Foundation of Korea, NRF; Instituto Nazionale di Fisica Nucleare, INFN; Norsk Sykepleierforbund, NSF; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, FAPERJ; Ministério da Educação, MEC; Bundesministerium für Bildung und Frauen, BMBF; European Regional Development Fund, ERDF; Department of Science and Technology, Government of West Bengal, DSTen_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.relation.ispartofPhysical Review Den_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subject[No Keyword Available]en_US
dc.titleSearch for Top Squarks and Dark Matter Particles in Opposite-Charge Dilepton Final States at S = 13 Teven_US
dc.typeArticleen_US
dc.institutionauthorKarapınar, Güler-
dc.departmentIzmir Institute of Technologyen_US
dc.identifier.volume97en_US
dc.identifier.issue3en_US
dc.identifier.wosWOS:000425093700001-
dc.identifier.wosWOS:000425093700001-
dc.identifier.scopus2-s2.0-85043365002-
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.identifier.doi10.1103/PhysRevD.97.032009-
dc.relation.doi10.1103/PhysRevD.97.032009en_US
dc.coverage.doi10.1103/PhysRevD.97.032009-
dc.authorscopusid16239550900-
dc.authorscopusid35222495600-
dc.authorscopusid56217303000-
dc.authorscopusid57195404626-
dc.authorscopusid55175601800-
dc.authorscopusid56236454000-
dc.authorscopusid57094679500-
dc.identifier.wosqualityQ1-
dc.identifier.scopusqualityQ1-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.openairetypeArticle-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.grantfulltextnone-
item.fulltextNo Fulltext-
Appears in Collections:Rectorate / Rektörlük
Scopus İndeksli Yayınlar Koleksiyonu / Scopus Indexed Publications Collection
WoS İndeksli Yayınlar Koleksiyonu / WoS Indexed Publications Collection
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