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Wh plus missing-ET signature from gaugino pair production at the LHC

Howard Baer1, Vernon Barger2, Andre Lessa3, Warintorn Sreethawong1, and Xerxes Tata4

  • 1Department of Physics and Astronomy, University of Oklahoma, Norman, Oklahoma, 73019, USA
  • 2Department of Physics, University of Wisconsin, Madison, Wisconsin 53706, USA
  • 3Instituto de Física, Universidade de São Paulo, São Paulo - SP, Brazil
  • 4Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA

Phys. Rev. D 85, 055022 – Published 23 March, 2012

DOI: https://doi.org/10.1103/PhysRevD.85.055022

Abstract

In SUSY models with heavy squarks and gaugino mass unification, the gaugino pair production reaction ppW˜1±Z˜2 dominates gluino pair production for mg˜1TeV at LHC with s=14TeV (LHC14). For this mass range, the two-body decays W˜1WZ˜1 and Z˜2hZ˜1 are expected to dominate the chargino and neutralino branching fractions. By searching for bb˜+T events from W˜1±Z˜2 production, we show that LHC14 with 100fb1 of integrated luminosity becomes sensitive to chargino masses in the range mW˜1450550GeV corresponding to mg˜1.52TeV in models with gaugino mass unification. For 103fb1, LHC14 is sensitive to the Wh channel for mW˜1300800GeV, corresponding to mg˜12.8TeV, which is comparable to the reach for gluino pair production followed by cascade decays. The Wh+T search channel opens up a new complementary avenue for SUSY searches at LHC, and serves to point to SUSY as the origin of any new physics discovered via multijet and multilepton +T channels.

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