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dc.contributorCMS Collaboration
dc.contributor.otherCMS Collaboration (ukupan broj autora: 2337)
dc.creatorSirunyan, A. M.
dc.creatorTumasyan, A.
dc.creatorAdam, W.
dc.creatorAmbrogi, F.
dc.creatorBergauer, T.
dc.creatorAdžić, Petar
dc.creatorĆirković, Predrag
dc.creatorĐorđević, Miloš
dc.creatorMilenović, Predrag
dc.creatorMilošević, Jovan
dc.creatorStojanović, Milan
dc.date.accessioned2020-07-30T11:43:27Z
dc.date.available2020-07-30T11:43:27Z
dc.date.issued2019
dc.identifier.issn2470-0010
dc.identifier.urihttps://vinar.vin.bg.ac.rs/handle/123456789/8761
dc.description.abstractA search for long-lived particles decaying to photons and weakly interacting particles, using proton-proton collision data at s=13 TeV collected by the CMS experiment in 2016–2017 is presented. The data set corresponds to an integrated luminosity of 77.4 fb−1. Results are interpreted in the context of supersymmetry with gauge-mediated supersymmetry breaking, where the neutralino is long-lived and decays to a photon and a gravitino. Limits are presented as a function of the neutralino proper decay length and mass. For neutralino proper decay lengths of 0.1, 1, 10, and 100 m, masses up to 320, 525, 360, and 215 GeV are excluded at 95% confidence level, respectively. We extend the previous best limits in the neutralino proper decay length by up to one order of magnitude, and in the neutralino mass by up to 100 GeV.en
dc.language.isoen
dc.rightsopenAccess
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.sourcePhysical Review D
dc.titleSearch for long-lived particles using delayed photons in proton-proton collisions at s=13 TeVen
dc.typearticleen
dc.rights.licenseBY
dcterms.abstractЦМС Цоллаборатион (укупан број аутора: 2337); Тумасyан, A.; Aдам, W.; Aмброги, Ф.; Бергауер, Т.; Aдзиц, П.; Цирковиц, П.; Дордевиц, М.; Миленовиц, П.; Милосевиц, Ј.; Стојановиц, М.; Сирунyан, A. М.;
dc.rights.holder© 2019 CERN. for the CMS Collaboration
dc.citation.volume100
dc.citation.issue11
dc.identifier.wos000501488800001
dc.identifier.doi10.1103/PhysRevD.100.112003
dc.citation.rankM21
dc.type.versionpublishedVersion
dc.identifier.scopus2-s2.0-85076552469
dc.identifier.fulltexthttps://vinar.vin.bg.ac.rs/bitstream/id/21708/PhysRevD.100.112003.pdf


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