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dc.contributor.authorSirunyan, A. M.
dc.contributor.authorSanders, Stephen J.
dc.contributor.authorCMS Collaboration
dc.date.accessioned2021-01-27T21:49:13Z
dc.date.available2021-01-27T21:49:13Z
dc.date.issued2019-01-10
dc.identifier.citationA. M. Sirunyan et al., "Search for Dark Matter Particles Produced in Association with a Top Quark Pair at √s = 13  TeV", Phys. Rev. Lett. 122, 011803, 10 January 2019, American Physical Society, https://doi.org/10.1103/PhysRevLett.122.011803en_US
dc.identifier.urihttp://hdl.handle.net/1808/31288
dc.descriptionThis work is licensed under a Creative Commons Attribution 4.0 International License.en_US
dc.description.abstractA search is performed for dark matter particles produced in association with a top quark pair in proton-proton collisions at √s=13 TeV. The data correspond to an integrated luminosity of 35.9 fb−1 recorded by the CMS detector at the LHC. No significant excess over the standard model expectation is observed. The results are interpreted using simplified models of dark matter production via spin-0 mediators that couple to dark matter particles and to standard model quarks, providing constraints on the coupling strength between the mediator and the quarks. These are the most stringent collider limits to date for scalar mediators, and the most stringent for pseudoscalar mediators at low masses.en_US
dc.publisherAmerican Physical Societyen_US
dc.rights© 2019 CERN, for the CMS Collaboration.en_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_US
dc.titleSearch for Dark Matter Particles Produced in Association with a Top Quark Pair at √s = 13  TeVen_US
dc.typeArticleen_US
kusw.kuauthorSanders, Stephen J.
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1103/PhysRevLett.122.011803en_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 CERN, for the CMS Collaboration.
Except where otherwise noted, this item's license is described as: © 2019 CERN, for the CMS Collaboration.