Phenomenology of Gluino Searches at the Tevatron

dc.creatorHaber, Howard E.
dc.date1993-08-06
dc.date.accessioned2026-07-07T03:56:18Z
dc.date.available2026-07-07T03:56:18Z
dc.descriptionPresent data indicates that the gluino (if it exists) must be heavier than about 95~GeV. During the next few years as the Tevatron integrated luminosity increases, gluino searches will be able to probe the mass range between 100 and 200~GeV. For masses in this range, a variety of gluino decay modes can provide viable signatures for gluino detection. Apart from the classic missing transverse energy signal, the detection of high transverse momentum like-sign dileptons may be the cleanest signature for gluino production. Other signatures such as the production of a hard photon in the gluino cascade decay may also play an important role in confirming the supersymmetric origin of events originating from gluino production and decay.
dc.description17 pages, PHYZZX format (with Ray Cowan's TABLES.TEX macros), invited talk presented at the SUSY-93 Workshop, Northeastern University, Boston, MA, 29 March--1 April 1993
dc.identifierhttps://arxiv.org/abs/hep-ph/9308235
dc.identifierhttp://arxiv.org/abs/hep-ph/9308235
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44911
dc.subjectHigh Energy Physics - Phenomenology
dc.titlePhenomenology of Gluino Searches at the Tevatron
dc.typetext

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