Light Gluino And Tevatroin Dijet Angular Distributions

dc.creatorTerekhov, Igor V.
dc.date1997-02-11
dc.date.accessioned2026-07-07T10:33:28Z
dc.date.available2026-07-07T10:33:28Z
dc.descriptionWe consider the effects of a light gluino on the dijet angular distributions in p - pbar collisions at sqrt(s)=1800 GeV. We show that the slower running of alpha_s and the production q qbar, g g -> Gino Gino do not significantly alter the expected angular distributions. On the other hand, single U, D squark production q g -> Q Gino with subsequent Q -> q g results in dijets whose angular distributions are dramatically different from that in SM. The CDF data on dijet angular distributions with integrated luminosity of 106 pb^(-1) exclude U, D squarks in the mass ranges 170 < m < 650 and 190 < m < 600 GeV, We consider lower energies as well and show that in a future experimental analysis for dijet mass below 240 GeV squarks could be observed or ruled out.
dc.description10 pages, LaTeX with 2 epsf figures
dc.identifierhttps://arxiv.org/abs/hep-ph/9702301
dc.identifierhttp://arxiv.org/abs/hep-ph/9702301
dc.identifierPhys.Lett.B412:86-90,1997
dc.identifierdoi:10.1016/S0370-2693(97)01063-0
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179119
dc.subjectHigh Energy Physics - Phenomenology
dc.titleLight Gluino And Tevatroin Dijet Angular Distributions
dc.typetext

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