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dc.contributor.authorChatrchyan, S.A.
dc.contributor.authorKhachatryan, Vladimir A.
dc.contributor.authorSirunyan, A.M.
dc.contributor.authorTumasyan, A.R.
dc.contributor.authorBaarmand, Marc M.
dc.contributor.authorDorney, B.
dc.contributor.authorHohlmann, Marcus
dc.contributor.authorKalakhety, Himali
dc.contributor.authorVodopiyanov, Igor
dc.contributor.authorYumiceva, Francisco
dc.date.accessioned2013-11-19T14:15:02Z
dc.date.available2013-11-19T14:15:02Z
dc.date.issued2013-03-26
dc.identifier.citationChatrchyan, S., Khachatryan, V., Sirunyan, A. M., Tumasyan, A., Adam, W., Aguilo, E., . . . Swanson, J. (2013). Search for contact interactions using the inclusive jet pT spectrum in pp collisions at √s=7 TeV. Physical Review D - Particles, Fields, Gravitation and Cosmology, 87(5)en_US
dc.identifier.urihttp://hdl.handle.net/11141/179
dc.description.abstractResults are reported of a search for a deviation in the jet production cross section from the prediction of perturbative quantum chromodynamics at next-to-leading order. The search is conducted using a 7 TeV proton-proton data sample corresponding to an integrated luminosity of 5.0 fb-1, collected with the Compact Muon Solenoid detector at the Large Hadron Collider. A deviation could arise from interactions characterized by a mass scale Λ too high to be probed directly at the LHC. Such phenomena can be modeled as contact interactions. No evidence of a deviation is found. Using the CL s criterion, lower limits are set on Λ of 9.9 TeV and 14.3 TeV at 95% confidence level for models with destructive and constructive interference, respectively. Limits obtained with a Bayesian method are also reported.en_US
dc.language.isoen_USen_US
dc.rightsThis published article is available in accordance with the publisher's policy. It may be subject to U.S. copyright law.en_US
dc.rights.urihttp://publish.aps.org/authors/transfer-of-copyright-agreementen_US
dc.titleSearch for contact interactions using the inclusive jet pT spectrum in pp collisions at √s=7 TeVen_US
dc.typeArticleen_US
dc.identifier.doi10.1103/PhysRevD.87.052017


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