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  4. Search for Excited Quarks of Light and Heavy Flavor in γ  + Jet Final States in Proton–proton Collisions at √s = 13 TeV

Search for Excited Quarks of Light and Heavy Flavor in γ  + Jet Final States in Proton–proton Collisions at √s = 13 TeV

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Author(s)
CMS Collaboration
•
Abercrombie, Daniel Robert
•
Allen, Brandon Leigh
•
Azzolini, Virginia
•
Barbieri, Richard Alexander
•
Baty, Austin Alan
•
Bi, Ran
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Brandt, Stephanie Akemi
•
Busza, Wit
•
Cali, Ivan Amos
more
Date Issued
April 2018
Journal
Physics Letters B
Publisher
Elsevier
Citation
Sirunyan, A.M. et al. “Search for Excited Quarks of Light and Heavy Flavor in γ  + Jet Final States in Proton–proton Collisions at √s = 13 TeV.” Physics Letters B 781 (June 2018): 390–411 © 2018 The Author(s)
Version
Final published version
Abstract
A search is presented for excited quarks of light and heavy flavor that decay to γ+jet final states. The analysis is based on data corresponding to an integrated luminosity of 35.9fb⁻¹ collected by the CMS experiment in proton–proton collisions at √s = 13 TeV at the LHC. A signal would appear as a resonant contribution to the invariant mass spectrum of the γ+jet system, above the background expected from standard model processes. No resonant excess is found, and upper limits are set on the product of the excited quark cross section and its branching fraction as a function of its mass. These are the most stringent limits to date in the γ+jet final state, and exclude excited light quarks with masses below 5.5 TeV and excited b quarks with masses below 1.8 TeV, assuming standard model like coupling strengths. Keywords: CMS; Physics; Excited quarks
MIT Department
Massachusetts Institute of Technology. Department of Nuclear Science and Engineering
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Laboratory for Nuclear Science
Terms of Use
Creative Commons Attribution 4.0 International License
http://creativecommons.org/licenses/by/4.0/
Persistent DSpace Link
http://hdl.handle.net/1721.1/118972
DOI of Published Version
https://doi.org/10.1016/J.PHYSLETB.2018.04.007
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