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High mass exclusive diffractive dijet production in ppbar collisions at √s = 1.96 TeV

dc.contributor.authorBaringer, Philip S.
dc.contributor.authorBean, Alice
dc.contributor.authorChen, G.
dc.contributor.authorClutter, Justace Randall
dc.contributor.authorMcGivern, Carrie Lynne
dc.contributor.authorSekaric, Jadranka
dc.contributor.authorWilson, Graham Wallace
dc.contributor.authorD0 Collaboration
dc.contributor.authorAbazov, V. M.
dc.contributor.authorAbbott, B.
dc.contributor.authorAbolins, M.
dc.contributor.authorAcharya, B. S.
dc.contributor.authorAdams, M.
dc.contributor.authorAdams, T.
dc.date.accessioned2015-05-26T19:03:08Z
dc.date.available2015-05-26T19:03:08Z
dc.date.issued2011-11-11
dc.identifier.citationAbazov, V.M. et al. (2011). "High mass exclusive diffractive dijet production in ppbar collisions at √s = 1.96 TeV." Physics Letters B, 705(3):193-199. http://www.dx.doi.org/10.1016/j.physletb.2011.10.013.en_US
dc.identifier.urihttp://hdl.handle.net/1808/17838
dc.description.abstractWe present evidence for diffractive exclusive dijet production with an invariant dijet mass greater than 100 GeV in data collected with the D0 experiment at the Fermilab Tevatron Collider. A discriminant based on calorimeter information is used to measure a significant number of events with little energy (typically less than 10 GeV) outside the dijet system, consistent with the diffractive exclusive dijet production topology. The probability for these events to be explained by other dijet production processes is 2×^(10−6), corresponding to a 4.7 standard deviation significance.en_US
dc.publisherElsevier: SCOAP3en_US
dc.rightsThis article is published by Elsevier under a Creative Commons Attribution License, and is available electronically from http://www.sciencedirect.com/science/article/pii/S0370269311012457.
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.titleHigh mass exclusive diffractive dijet production in ppbar collisions at √s = 1.96 TeVen_US
dc.typeArticle
kusw.kuauthorBaringer, Philip S.
kusw.kuauthorBean, Alice
kusw.kuauthorChen, G.
kusw.kuauthorClutter, Justace Randall
kusw.kuauthorMcGivern, Carrie Lynne
kusw.kuauthorSekaric, Jadranka
kusw.kuauthorWilson, Graham Wallace
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1016/j.physletb.2011.10.013
kusw.oaversionScholarly/refereed, publisher version
kusw.oapolicyThis item meets KU Open Access policy criteria.
dc.rights.accessrightsopenAccess


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This article is published by Elsevier under a Creative Commons Attribution License, and is available electronically from http://www.sciencedirect.com/science/article/pii/S0370269311012457.
Except where otherwise noted, this item's license is described as: This article is published by Elsevier under a Creative Commons Attribution License, and is available electronically from http://www.sciencedirect.com/science/article/pii/S0370269311012457.