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  4. Search for the supersymmetric partner of the top quark in pp̅ collisions at √s=1.96  TeV

Search for the supersymmetric partner of the top quark in pp̅ collisions at √s=1.96  TeV

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Author(s)
Gomez-Ceballos, Guillelmo
•
Goncharov, Maxim
•
Makhoul, Khaldoun
•
Paus, Christoph M. E.
•
Bauer, Gerry P
Date Issued
November 2010
Journal
Physical Review D
Publisher
American Physical Society
Citation
Aaltonen, T. et al. “Search for the supersymmetric partner of the top quark in pp[over ¯] collisions at sqrt[s]=1.96  TeV.” Physical Review D 82.9 (2010) : n. pag. © 2010 The American Physical Society
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Final published version
Abstract
We present a search for the lightest supersymmetric partner of the top quark in proton-antiproton collisions at a center-of-mass energy √s=1.96  [square root of s-1.96] TeV. This search was conducted within the framework of the R parity conserving minimal supersymmetric extension of the standard model, assuming the stop decays dominantly to a lepton, a sneutrino, and a bottom quark. We searched for events with two oppositely-charged leptons, at least one jet, and missing transverse energy in a data sample corresponding to an integrated luminosity of 1  fb-1 [fb superscript -1] collected by the Collider Detector at Fermilab experiment. No significant evidence of a stop quark signal was found. Exclusion limits at 95% confidence level in the stop quark versus sneutrino mass plane are set. Stop quark masses up to 180  GeV/c2 [GeV/c superscript 2] are excluded for sneutrino masses around 45  GeV/c2 [GeV/c superscript 2], and sneutrino masses up to 116  GeV/c2 [GeV/c superscript 2] are excluded for stop quark masses around 150  GeV/c2 [GeV/c superscript 2].
MIT Department
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Laboratory for Nuclear Science
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Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
http://hdl.handle.net/1721.1/62848
DOI of Published Version
https://doi.org/10.1103/PhysRevD.82.092001
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