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dc.contributor.authorCMS Collaboration
dc.date.accessioned2017-10-25T18:26:28Z
dc.date.available2017-10-25T18:26:28Z
dc.date.issued2016-02-10
dc.identifier.citationKhachatryan, V., Erbacher, R., Carrillo Montoya, C. A., Carvalho, W., Górski, M., Kotlinski, D., ... & Lander, R. (2015). Search for a Higgs boson decaying into $\gamma^*\gamma\to\ell\ell\gamma $ with low dilepton mass in pp collisions at $\sqrt s= $8 TeV. Phys. Lett., 753(CMS-HIG-14-003), 341-362.en_US
dc.identifier.urihttp://hdl.handle.net/1808/25192
dc.description.abstractA search is described for a Higgs boson decaying into two photons, one of which has an internal conversion to a muon or an electron pair (ℓℓγ). The analysis is performed using proton–proton collision data recorded with the CMS detector at the LHC at a centre-of-mass energy of 8 TeV, corresponding to an integrated luminosity of 19.7 fb−1. The events selected have an opposite-sign muon or electron pair and a high transverse momentum photon. No excess above background has been found in the three-body invariant mass range 120<mℓℓγ<150 GeV120<mℓℓγ<150 GeV, and limits have been derived for the Higgs boson production cross section times branching fraction for the decay H→γ⁎γ→ℓℓγH→γ⁎γ→ℓℓγ, where the dilepton invariant mass is less than 20 GeV. For a Higgs boson with mH=125 GeVmH=125 GeV, a 95% confidence level (CL) exclusion observed (expected) limit is 6.7 (View the MathML source5.9−1.8+2.8) times the standard model prediction. Additionally, an upper limit at 95% CL on the branching fraction of H→(J/ψ)γH→(J/ψ)γ for the 125 GeV Higgs boson is set at 1.5×10−31.5×10−3.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.en_US
dc.subjectCMSen_US
dc.subjectPhysicsen_US
dc.subjectHiggs bosonen_US
dc.subjectDalitz decayen_US
dc.titleSearch for a Higgs boson decaying into γ⁎ γ→ ℓℓγ with low dilepton mass in pp collisions aten_US
dc.typeArticleen_US
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1016/j.physletb.2015.12.039en_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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