Show simple item record

dc.contributor.authorSirunyan, A.M.
dc.contributor.authorSanders, Stephen J.
dc.contributor.authorThe CMS Collaboration
dc.date.accessioned2021-01-26T19:51:41Z
dc.date.available2021-01-26T19:51:41Z
dc.date.issued2019-11-10
dc.identifier.citationA.M. Sirunyan et al., "Combination of CMS searches for heavy resonances decaying to pairs of bosons or leptons", Physics Letters B, Volume 798, 2019, 134952, ISSN 0370-2693, https://doi.org/10.1016/j.physletb.2019.134952. (http://www.sciencedirect.com/science/article/pii/S0370269319306744)en_US
dc.identifier.urihttp://hdl.handle.net/1808/31256
dc.descriptionThis work is licensed under a Creative Commons Attribution 4.0 International License.en_US
dc.description.abstractA statistical combination of searches for heavy resonances decaying to pairs of bosons or leptons is presented. The data correspond to an integrated luminosity of 35.9 fb−1 collected during 2016 by the CMS experiment at the LHC in proton-proton collisions at a center-of-mass energy of 13 TeV. The data are found to be consistent with expectations from the standard model background. Exclusion limits are set in the context of models of spin-1 heavy vector triplets and of spin-2 bulk gravitons. For massdegenerate W and Z resonances that predominantly couple to the standard model gauge bosons, the mass exclusion at 95% confidence level of heavy vector bosons is extended to 4.5 TeV as compared to 3.8 TeV determined from the best individual channel. This excluded mass increases to 5.0 TeV if the resonances couple predominantly to fermions.en_US
dc.publisherElsevieren_US
dc.rights© 2019 The Author(s). Published by Elsevier B.V.en_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_US
dc.subjectCMSen_US
dc.subjectB2Gen_US
dc.subjectDibosonen_US
dc.subjectDileptonen_US
dc.subjectHVTen_US
dc.subjectGravitonen_US
dc.titleCombination of CMS searches for heavy resonances decaying to pairs of bosons or leptonsen_US
dc.typeArticleen_US
kusw.kuauthorSanders, Stephen J.
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1016/j.physletb.2019.134952en_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.rights.accessrightsopenAccessen_US


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record

© 2019 The Author(s). Published by Elsevier B.V.
Except where otherwise noted, this item's license is described as: © 2019 The Author(s). Published by Elsevier B.V.