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dc.contributor.authorSirunyan, A. M.
dc.contributor.authorSanders, Stephen J.
dc.contributor.authorThe CMS collaboration
dc.date.accessioned2021-01-15T19:19:57Z
dc.date.available2021-01-15T19:19:57Z
dc.date.issued2019-04-03
dc.identifier.citationThe CMS collaboration., Sirunyan, A.M., Tumasyan, A. et al. Search for resonant tt production in proton-proton collisions at √𝑠=13 TeV. J. High Energ. Phys. 2019, 31 (2019). https://doi.org/10.1007/JHEP04(2019)031en_US
dc.identifier.urihttp://hdl.handle.net/1808/31151
dc.descriptionThis work is licensed under a Creative Commons Attribution 4.0 International License.en_US
dc.description.abstractA search for a heavy resonance decaying into a top quark and antiquark (tt) pair is performed using proton-proton collisions at √𝑠=13 TeV. The search uses the data set collected with the CMS detector in 2016, which corresponds to an integrated luminosity of 35.9 fb−1. The analysis considers three exclusive final states and uses reconstruction techniques that are optimized for top quarks with high Lorentz boosts, which requires the use of nonisolated leptons and jet substructure techniques. No significant excess of events relative to the expected yield from standard model processes is observed. Upper limits on the production cross section of heavy resonances decaying to a tt pair are calculated. Limits are derived for a leptophobic topcolor Z′ resonance with widths of 1, 10, and 30%, relative to the mass of the resonance, and exclude masses up to 3.80, 5.25, and 6.65 TeV, respectively. Kaluza-Klein excitations of the gluon in the Randall-Sundrum model are excluded up to 4.55 TeV. To date, these are the most stringent limits on tt resonances.en_US
dc.publisherSpringer Verlagen_US
dc.rightsCopyright CERN, for the benefit of the CMS Collaboration.en_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_US
dc.subjectBeyond Standard Modelen_US
dc.subjectHadron-Hadron scattering (experiments)en_US
dc.titleSearch for resonant tt production in proton-proton collisions at √𝑠=13 TeVen_US
dc.typeArticleen_US
kusw.kuauthorSanders, Stephen J.
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1007/JHEP04(2019)031en_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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Copyright CERN, for the benefit of the CMS Collaboration.
Except where otherwise noted, this item's license is described as: Copyright CERN, for the benefit of the CMS Collaboration.