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  4. Search for Evidence of the Type-III Seesaw Mechanism in Multilepton Final States in Proton-Proton Collisions at √s = 13 TeV

Search for Evidence of the Type-III Seesaw Mechanism in Multilepton Final States in Proton-Proton Collisions at √s = 13 TeV

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Author(s)
CMS Collaboration
•
Abercrombie, Daniel Robert
•
Allen, Brandon Leigh
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Azzolini, Virginia
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Barbieri, Richard Alexander
•
Baty, Austin Alan
•
Bi, Ran
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Brandt, Stephanie Akemi
•
Busza, Wit
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Cali, Ivan Amos
more
Date Issued
December 2017
Journal
Physical Review Letters
Publisher
American Physical Society
Citation
Sirunyan, A. M. et al. “Search for Evidence of the Type-III Seesaw Mechanism in Multilepton Final States in Proton-Proton Collisions at √s = 13 TeV.” Physical Review Letters 119, 22 (December 2017): 221802 © 2017 CERN, for the CMS Collaboration
Version
Final published version
Abstract
A search for a signal consistent with the type-III seesaw mechanism in events with three or more electrons or muons is presented. The data sample consists of proton-proton collisions at √s=13  TeV collected by the CMS experiment at the LHC in 2016 and corresponds to an integrated luminosity of 35.9  fb[superscript −1]. Selection criteria based on the number of leptons and the invariant mass of oppositely charged lepton pairs are used to distinguish the signal from the standard model background. The observations are consistent with the expectations from standard model processes. The results are used to place limits on the production of heavy fermions of the type-III seesaw model as a function of the branching ratio to each lepton flavor. In the scenario of equal branching fractions to each lepton flavor, heavy fermions with masses below 840 GeV are excluded. This is the most sensitive probe to date of the type-III seesaw mechanism.
MIT Department
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Laboratory for Nuclear Science
Terms of Use
Creative Commons Attribution 3.0 Unported license
http://creativecommons.org/licenses/by/3.0/
Persistent DSpace Link
http://hdl.handle.net/1721.1/114598
DOI of Published Version
https://doi.org/10.1103/PhysRevLett.119.221802
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