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dc.contributor.authorBaringer, Philip S.
dc.contributor.authorBean, Alice
dc.contributor.authorMurray, Michael J.
dc.contributor.authorSanders, Stephen J.
dc.date.accessioned2016-12-07T18:01:20Z
dc.date.available2016-12-07T18:01:20Z
dc.date.issued2015-04-13
dc.identifier.citationSearches for supersymmetry based on events with b jets and four W bosons in pp collisions at 8 TeV. (2015). Physics Letters B, 745, 5–28. doi:10.1016/j.physletb.2015.04.002en_US
dc.identifier.urihttp://hdl.handle.net/1808/22164
dc.description.abstractFive mutually exclusive searches for supersymmetry are presented based on events in which b jetsb jets and four W bosons are produced in proton–proton collisions at View the MathML sources=8 TeV. The data, corresponding to an integrated luminosity of 19.5 fb−119.5 fb−1, were collected with the CMS experiment at the CERN LHC in 2012. The five studies differ in the leptonic signature from the W boson decays, and correspond to all-hadronic, single-lepton, opposite-sign dilepton, same-sign dilepton, and ≥3 lepton final states. The results of the five studies are combined to yield 95% confidence level limits for the gluino and bottom-squark masses in the context of gluino and bottom-squark pair production, respectively. In the limit when the lightest supersymmetric particle is light, gluino and bottom squark masses are excluded below 1280 and 570 GeV570 GeV, respectively.en_US
dc.publisherElsevieren_US
dc.rights©2015 CERN for the benefit of the CMS Collaboration. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP3.en_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subjectCMSen_US
dc.subjectPhysicsen_US
dc.subjectSupersymmetryen_US
dc.titleSearches for supersymmetry based on events with b jets and four W bosons in pp collisions at 8 TeVen_US
dc.typeArticleen_US
kusw.kuauthorBaringer, Philip S.
kusw.kuauthorBean, Alice
kusw.kuauthorMurray, Michael J.
kusw.kuauthorSanders, Stephen J.
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1016/j.physletb.2015.04.002en_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.rights.accessrightsopenAccess


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©2015 CERN for the benefit of the CMS Collaboration. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP3.
Except where otherwise noted, this item's license is described as: ©2015 CERN for the benefit of the CMS Collaboration. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP3.