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Search for Dark Matter Particles Produced in Association with a Top Quark Pair at √s =13 TeV

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dc.contributor.author CMS Collaboration en_US
dc.contributor.author Sirunyan, A. M. en_US
dc.contributor.author CHAUHAN, S. en_US
dc.contributor.author DUBE, SOURABH en_US
dc.contributor.author HEGDE, V. en_US
dc.contributor.author KAPOOR, A. en_US
dc.contributor.author KOTHEKAR, K. en_US
dc.contributor.author PANDEY, S. en_US
dc.contributor.author RANE, A. en_US
dc.contributor.author SHARMA, SEEMA et al. en_US
dc.date.accessioned 2019-02-01T05:10:33Z
dc.date.available 2019-02-01T05:10:33Z
dc.date.issued 2019-01 en_US
dc.identifier.citation Physical Review Letters, 122(1). en_US
dc.identifier.issn 0031-9007 en_US
dc.identifier.issn 1079-7114 en_US
dc.identifier.uri http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/1572
dc.identifier.uri https://doi.org/10.1103/PhysRevLett.122.011803 en_US
dc.description.abstract A search is performed for dark matter particles produced in association with a top quark pair in proton-proton collisions at root 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.language.iso en en_US
dc.publisher American Physical Society en_US
dc.subject Candidates en_US
dc.subject TOC-JAN-2019 en_US
dc.subject 2019 en_US
dc.title Search for Dark Matter Particles Produced in Association with a Top Quark Pair at √s =13 TeV en_US
dc.type Article en_US
dc.contributor.department Dept. of Physics en_US
dc.identifier.sourcetitle Physical Review Letters en_US
dc.publication.originofpublisher Foreign en_US


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