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  4. A search for pair production of new light bosons decaying into muons in proton-proton collisions at 13 TeV

A search for pair production of new light bosons decaying into muons in proton-proton collisions at 13 TeV

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sword-2020-02-14T18:39:48.original.xml (130 B)
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Author(s)
CMS Collaboration
•
Benvenuti, A. C.
•
Chatterjee, R.M.
•
Evans, A.
•
Hansen, P.
•
Hiltbrand, J.
•
Jain, Sh.
•
Kalafut, S.
•
Krohn, M.
•
Kubota, Yasuo
more
Date Issued
September 2019
Journal
Physics Letters B
Publisher
Elsevier BV
Citation
CMS Collaboration (Sirunyan, A.M., et al.), "A search for pair production of new light bosons decaying into muons in proton-proton collisions at 13 TeV." Physics Letters B 796 (Sept. 2019): p. 131-54 doi 10.1016/J.PHYSLETB.2019.07.013 ©2019 Author(s)
Version
Final published version
Abstract
A search for new light bosons decaying into muon pairs is presented using a data sample corresponding to an integrated luminosity of 35.9fb−1 of proton-proton collisions at a center-of-mass energy s=13TeV, collected with the CMS detector at the CERN LHC. The search is model independent, only requiring the pair production of a new light boson and its subsequent decay to a pair of muons. No significant deviation from the predicted background is observed. A model independent limit is set on the product of the production cross section times branching fraction to dimuons squared times acceptance as a function of new light boson mass. This limit varies between 0.15 and 0.39 fb over a range of new light boson masses from 0.25 to 8.5 GeV. It is then interpreted in the context of the next-to-minimal supersymmetric standard model and a dark supersymmetry model that allows for nonnegligible light boson lifetimes. In both cases, there is significant improvement over previously published limits. ©2019
MIT Department
Massachusetts Institute of Technology. Department of Physics
Terms of Use
Creative Commons Attribution 4.0 International license
https://creativecommons.org/licenses/by/4.0/
Persistent DSpace Link
https://hdl.handle.net/1721.1/125024
DOI of Published Version
https://doi.org/10.1016/J.PHYSLETB.2019.07.013
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