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dc.contributor.authorCMS Collaboration
dc.date.accessioned2022-05-03T15:23:39Z
dc.date.available2022-05-03T15:23:39Z
dc.date.issued2022-02-17
dc.identifier.citationTumasyan, A., Adam, W., Andrejkovic, J.W. et al. Search for long-lived particles decaying to leptons with large impact parameter in proton–proton collisions at s√=13TeV. Eur. Phys. J. C 82, 153 (2022). https://doi.org/10.1140/epjc/s10052-022-10027-3en_US
dc.identifier.urihttp://hdl.handle.net/1808/32742
dc.description.abstractA search for new long-lived particles decaying to leptons using proton–proton collision data produced by the CERN LHC at s√=13TeV is presented. Events are selected with two leptons (an electron and a muon, two electrons, or two muons) that both have transverse impact parameter values between 0.01 and 10cm and are not required to form a common vertex. Data used for the analysis were collected with the CMS detector in 2016, 2017, and 2018, and correspond to an integrated luminosity of 118 (113)fb−1 in the ee channel (eμ and μμ channels). The search is designed to be sensitive to a wide range of models with displaced eμ, ee, and μμ final states. The results constrain several well-motivated models involving new long-lived particles that decay to displaced leptons. For some areas of the available phase space, these are the most stringent constraints to date.en_US
dc.publisherPublic Library of Scienceen_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 long-lived particles decaying to leptons with large impact parameter in proton–proton collisions at √s=13TeVen_US
dc.typeArticleen_US
kusw.kuauthorAbreu, A.
kusw.kuauthorAnguiano, J.
kusw.kuauthorBaldenegro Barrera, C.
kusw.kuauthorBaringer, P.
kusw.kuauthorBean, A.
kusw.kuauthorBylinkin, A.
kusw.kuauthorFlowers, Z.
kusw.kuauthorIsidori, T.
kusw.kuauthorKhalil, S.
kusw.kuauthorKing, J.
kusw.kuauthorKrintiras, G.
kusw.kuauthorKropivnitskaya, A.
kusw.kuauthorLazarovits, M.
kusw.kuauthorLe Mahieu, C.
kusw.kuauthorLindsey, C.
kusw.kuauthorMarquez, J.
kusw.kuauthorMinafra, N.
kusw.kuauthorMurray, M.
kusw.kuauthorNickel, M.
kusw.kuauthorRogan, C.
kusw.kuauthorRoyon, C.
kusw.kuauthorSalvatico, R.
kusw.kuauthorSanders, S.
kusw.kuauthorSchmitz, E.
kusw.kuauthorSmith, C.
kusw.kuauthorTapia Takaki, J. D.
kusw.kuauthorWang, Q.
kusw.kuauthorWarner, Z.
kusw.kuauthorWilliams, J.
kusw.kuauthorWilson, G.
kusw.kudepartmentPhysics & Astronomyen_US
dc.identifier.doi10.1140/epjc/s10052-022-10027-3en_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.identifier.pmidPMC8854303en_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.