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dc.contributor.authorBaringer, Philip S.
dc.contributor.authorBean, Alice
dc.contributor.authorHensel, Carsten
dc.contributor.authorMoulik, Tania
dc.contributor.authorWilson, Graham Wallace
dc.contributor.authorAbazov, V. M.
dc.contributor.authorAbbott, B.
dc.contributor.authorAbolins, M.
dc.contributor.authorAcharya, B. S.
dc.contributor.authorAdams, M.
dc.date.accessioned2014-10-28T17:02:03Z
dc.date.available2014-10-28T17:02:03Z
dc.date.issued2008-05-12
dc.identifier.citationV. M. Abazov et al. (D0 Collaboration). (2008). "Search for excited electrons in pp-bar collisions at s√=1.96  TeV." Physical Review D, 77(9):091102. http://dx.doi.org/10.1103/PhysRevD.77.091102
dc.identifier.issn1550-7998
dc.identifier.urihttp://hdl.handle.net/1808/15418
dc.descriptionThis is the publisher's version, also available electronically from http://journals.aps.org/prd/abstract/10.1103/PhysRevD.77.091102.
dc.description.abstractWe present the results of a search for the production of an excited state of the electron, e*, in proton-antiproton collisions at s√=1.96  TeV. The data were collected with the D0 experiment at the Fermilab Tevatron Collider and correspond to an integrated luminosity of approximately 1  fb(−1). We search for e* in the process pp-bar→e*e, with the e* subsequently decaying to an electron plus photon. No excess above the standard model background is observed. Interpreting our data in the context of a model that describes e* production by four-fermion contact interactions and e* decay via electroweak processes, we set 95% C.L. upper limits on the production cross section ranging from 8.9 to 27 fb, depending on the mass of the excited electron. Choosing the scale for contact interactions to be Λ=1  TeV, excited electron masses below 756 GeV are excluded at the 95% C.L.
dc.publisherAmerican Physical Society
dc.titleSearch for excited electrons in pp-bar collisions at s√=1.96  TeV
dc.typeArticle
kusw.kuauthorBaringer, Philip S.
kusw.kuauthorBean, Alice
kusw.kuauthorHensel, Carsten
kusw.kuauthorMoulik, Tania
kusw.kuauthorWilson, Graham Wallace
kusw.kudepartmentPhysics and Astronomy
dc.identifier.doi10.1103/PhysRevD.77.091102
kusw.oaversionScholarly/refereed, publisher version
kusw.oapolicyThis item does not meet KU Open Access policy criteria.
dc.rights.accessrightsopenAccess


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