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dc.contributor.authorCMS Collaboration
dc.date.accessioned2022-05-02T15:34:04Z
dc.date.available2022-05-02T15:34:04Z
dc.date.issued2022-03-10
dc.identifier.citationTumasyan, A., Adam, W., Bergauer, T. et al. Search for strongly interacting massive particles generating trackless jets in proton–proton collisions at s√=13TeV. Eur. Phys. J. C 82, 213 (2022). https://doi.org/10.1140/epjc/s10052-022-10095-5en_US
dc.identifier.urihttp://hdl.handle.net/1808/32731
dc.description.abstractA search for dark matter in the form of strongly interacting massive particles (SIMPs) using the CMS detector at the LHC is presented. The SIMPs would be produced in pairs that manifest themselves as pairs of jets without tracks. The energy fraction of jets carried by charged particles is used as a key discriminator to suppress efficiently the large multijet background, and the remaining background is estimated directly from data. The search is performed using proton–proton collision data corresponding to an integrated luminosity of 16.1fb−1, collected with the CMS detector in 2016. No significant excess of events is observed above the expected background. For the simplified dark matter model under consideration, SIMPs with masses up to 100GeV are excluded and further sensitivity is explored towards higher masses.en_US
dc.publisherSpringerOpenen_US
dc.rights© CERN for the benefit of the CMS Collaboration 2022. This article is licensed under a Creative Commons Attribution 4.0 International License.en_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_US
dc.titleSearch for strongly interacting massive particles generating trackless jets in proton–proton collisions at √s=13TeVen_US
dc.typeArticleen_US
kusw.kuauthorBaringer, P.
kusw.kuauthorBean, A.
kusw.kuauthorBylinkin, A.
kusw.kuauthorIsidori, T.
kusw.kuauthorKhalil, S.
kusw.kuauthorKing, J.
kusw.kuauthorKrintiras, G.
kusw.kuauthorKropivnitskaya, A.
kusw.kuauthorLindsey, C.
kusw.kuauthorMinafra, N.
kusw.kuauthorMurray, M.
kusw.kuauthorRogan, C.
kusw.kuauthorRoyon, C.
kusw.kuauthorSanders, S.
kusw.kuauthorSchmitz, E.
kusw.kuauthorTapia Takaki, J. D.
kusw.kuauthorWang, Q.
kusw.kuauthorWilliams, J.
kusw.kuauthorWilson, G.
kusw.kudepartmentPhysics & Astronomyen_US
dc.identifier.doi10.1140/epjc/s10052-022-10095-5en_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.identifier.pmidPMC8913525en_US
dc.rights.accessrightsopenAccessen_US


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© CERN for the benefit of the CMS Collaboration 2022. This article is licensed under a Creative Commons Attribution 4.0 International License.
Except where otherwise noted, this item's license is described as: © CERN for the benefit of the CMS Collaboration 2022. This article is licensed under a Creative Commons Attribution 4.0 International License.