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dc.contributor.authorCMS Collaboration
dc.date.accessioned2018-10-09T18:17:15Z
dc.date.available2018-10-09T18:17:15Z
dc.date.issued2017
dc.identifier.citationCMS Collaboration, Combination of searches for heavy resonances decaying to WW, WZ, ZZ, WH, and ZH boson pairs in proton–proton collisions at √s = 8and13 TeV, Physics Letters B. https://doi.org/10.1016/j.physletb.2017.09.083en_US
dc.identifier.urihttp://hdl.handle.net/1808/26801
dc.description.abstractA statistical combination of searches is presented for massive resonances decaying to WW, WZ, ZZ, WH, and ZH boson pairs in proton–proton collision data collected by the CMS experiment at the LHC. The data were taken at centre-of-mass energies of 8 and 13 TeV, corresponding to respective integrated luminosities of 19.7 and up to 2.7 fb−1. The results are interpreted in the context of heavy vector triplet and singlet models that mimic properties of composite-Higgs models predicting W'and Z' bosons decaying to WZ, WW, WH, and ZH bosons. Amodelwith a bulk graviton that decays into WW and ZZ is also considered. This is the first combined search for WW, WZ, WH, and ZH resonances and yields lower limits on masses at 95% confidence level for W' and Z' singlets at 2.3 TeV, and for a triplet at 2.4 TeV. The limits on the production cross section of a narrow bulk graviton resonance with the curvature scale of the warped extra dimension ˜k = 0.5, in the mass range of 0.6 to 4.0 TeV, are the most stringent published to date.en_US
dc.publisherElsevieren_US
dc.rights© 2017 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY licenseen_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_US
dc.subjectCMSen_US
dc.subjectPhysicsen_US
dc.subjectDi-bosonen_US
dc.subjectResonancesen_US
dc.subjectCombinationen_US
dc.titleCombination of searches for heavy resonances decaying to WW, WZ, ZZ, WH, and ZH boson pairs in proton–proton collisions at √s = 8and13 TeVen_US
dc.typeArticleen_US
kusw.kuauthorBaringer, Philip S.
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doihttps://doi.org/10.1016/j.physletb.2017.09.083en_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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© 2017 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license
Except where otherwise noted, this item's license is described as: © 2017 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license