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dc.contributor.authorAaboud, M.
dc.contributor.authorRogan, Christopher
dc.contributor.authorThe ATLAS Collaboration
dc.date.accessioned2021-01-25T20:10:54Z
dc.date.available2021-01-25T20:10:54Z
dc.date.issued2019-03-10
dc.identifier.citationM. Aaboud et al., "Study of the hard double-parton scattering contribution to inclusive four-lepton production in pp collisions at s=8 TeV with the ATLAS detector", Physics Letters B, Volume 790, 2019, Pages 595-614, ISSN 0370-2693, https://doi.org/10.1016/j.physletb.2019.01.062. (http://www.sciencedirect.com/science/article/pii/S0370269319300875)en_US
dc.identifier.urihttp://hdl.handle.net/1808/31234
dc.descriptionThis work is licensed under a Creative Commons Attribution 4.0 International License.en_US
dc.description.abstractThe inclusive production of four isolated charged leptons in pp collisions is analysed for the presence of hard double-parton scattering, using 20.2 fb−1 of data recorded in the ATLAS detector at the LHC at centre-of-mass energy √s = 8 TeV. In the four-lepton invariant-mass range of 80 < m4 < 1000 GeV, an artificial neural network is used to enhance the separation between single- and double-parton scattering based on the kinematics of the four leptons in the final state. An upper limit on the fraction of events originating from double-parton scattering is determined at 95% confidence level to be fDPS = 0.042, which results in an estimated lower limit on the effective cross section at 95% confidence level of 1.0 mb.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.subjectFour-lepton productionen_US
dc.subjectDouble Drell–Yanen_US
dc.subjectDouble parton-scatteringen_US
dc.subjectHiggs golden decay channelen_US
dc.titleStudy of the hard double-parton scattering contribution to inclusive four-lepton production in pp collisions at √s = 8 TeV with the ATLAS detectoren_US
dc.typeArticleen_US
kusw.kuauthorRogan, Christopher
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1016/j.physletb.2019.01.062en_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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© 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.