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Search for Stopped Gluinos in pp Collisions at root s=7 TeV

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Author(s)
Alver, Burak Han
•
Bendavid, Joshua L.
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Busza, Wit
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Butz, Erik M.
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Cali, Ivan Amos
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Chan, M.
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Dutta, Valentina
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Everaerts, Pieter Bruno Bart
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Gomez-Ceballos, Guillelmo
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Goncharov, Maxim
more
Date Issued
January 2011
Journal
Physical review letters
Publisher
American Physical Society
Citation
Khachatryan, V. et al. "Search for Stopped Gluinos in pp Collisions at √s=7 [square root s=7] TeV" Physical review letters, v. 106, no. 1, Jan. 2011. © 2011 CERN, for the CMS Collaboration
Version
Final published version
Abstract
The results of the first search for long-lived gluinos produced in 7 TeV pp collisions at the CERN Large Hadron Collider are presented. The search looks for evidence of long-lived particles that stop in the CMS detector and decay in the quiescent periods between beam crossings. In a dataset with a peak instantaneous luminosity of 1×1032 [1 x 10 superscript 32]  cm-2 s-1 [cm superscript -2 s superscript -1] , an integrated luminosity of 10  pb-1 [pb superscript -1], and a search interval corresponding to 62 hours of LHC operation, no significant excess above background was observed. Limits at the 95% confidence level on gluino pair production over 13 orders of magnitude of gluino lifetime are set. For a mass difference mg˜-mχ˜10>100  GeV/c2 [m subscript _ g minus m subscript -0 over X subscript 1, greater than 100 GeV over c superscript 2], and assuming BR(g˜→gχ˜10)=100% [BR (g → g X -0 subscript 1 = 100%], mg˜<370  GeV/c2 [m subscript g less than 370 GeV over c superscript 2]are excluded for lifetimes from 10  μs [mu s] to 1000 s
MIT Department
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Laboratory for Nuclear Science
Terms of Use
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/1721.1/64413
DOI of Published Version
https://doi.org/10.1103/PhysRevLett.106.011801
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