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dc.contributor.authorCMS Collaboration
dc.date.accessioned2023-08-14T14:15:03Z
dc.date.available2023-08-14T14:15:03Z
dc.date.issued2023-07-26
dc.identifier.citationTumasyan, A., Adam, W., Andrejkovic, J.W. et al. Measurements of the Higgs boson production cross section and couplings in the W boson pair decay channel in proton-proton collisions at √𝑠=13TeV. Eur. Phys. J. C 83, 667 (2023). https://doi.org/10.1140/epjc/s10052-023-11632-6en_US
dc.identifier.urihttps://hdl.handle.net/1808/34723
dc.description.abstractProduction cross sections of the standard model Higgs boson decaying to a pair of W bosons are measured in proton-proton collisions at a center-of-mass energy of 13TeV. The analysis targets Higgs bosons produced via gluon fusion, vector boson fusion, and in association with a W or Z boson. Candidate events are required to have at least two charged leptons and moderate missing transverse momentum, targeting events with at least one leptonically decaying W boson originating from the Higgs boson. Results are presented in the form of inclusive and differential cross sections in the simplified template cross section framework, as well as couplings of the Higgs boson to vector bosons and fermions. The data set collected by the CMS detector during 2016–2018 is used, corresponding to an integrated luminosity of 138fb−1. The signal strength modifier 𝜇, defined as the ratio of the observed production rate in a given decay channel to the standard model expectation, is measured to be 𝜇=0.95+0.10−0.09. All results are found to be compatible with the standard model within the uncertainties.en_US
dc.publisherSpringerOpenen_US
dc.rights© CERN for the benefit of the CMS collaboration 2023. 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.titleMeasurements of the Higgs boson production cross section and couplings in the W boson pair decay channel in proton-proton collisions at √𝑠=13TeVen_US
dc.typeArticleen_US
kusw.kuauthorAbreu, A.
kusw.kuauthorAlcerro Alcerro, L. F.
kusw.kuauthorAnguiano, J.
kusw.kuauthorBaringer, P.
kusw.kuauthorBean, A.
kusw.kuauthorFlowers, Z.
kusw.kuauthorIsidori, T.
kusw.kuauthorKhalil, S.
kusw.kuauthorKing, J.
kusw.kuauthorKrintiras, G.
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.kuauthorSmith, C.
kusw.kuauthorWang, Q.
kusw.kuauthorWilliams, J.
kusw.kuauthorWilson, G.
kusw.kudepartmentPhysics & Astronomyen_US
dc.identifier.doi10.1140/epjc/s10052-023-11632-6en_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.rights.accessrightsopenAccessen_US


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© CERN for the benefit of the CMS collaboration 2023. 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 2023. This article is licensed under a Creative Commons Attribution 4.0 International License.