Testing SUSY models for the muon g2 anomaly via chargino-neutralino pair production at the LHC

Siba Prasad Das, Monoranjan Guchait, and D. P. Roy
Phys. Rev. D 90, 055011 – Published 10 September 2014

Abstract

Nonuniversal gaugino mass models can naturally account for the dark matter relic density via the bulk annihilation process with relatively light bino LSP and right sleptons in the mass range of 100  GeV, while accommodating the observed Higgs boson mass of 125  GeV with TeV scale squark/gluino masses. A class of these models can also account for the observed muon g-2 anomaly via SUSY loops with wino and left sleptons in the mass range of 400–700 GeV. These models can be tested at LHC via electroweak production of charged and neutral wino pair, leading to robust trilepton and same sign dilepton signals. We investigate these signals along with the standard model background for both 8 and 13 TeV LHC runs.

  • Received 22 July 2014

DOI:https://doi.org/10.1103/PhysRevD.90.055011

© 2014 American Physical Society

Authors & Affiliations

Siba Prasad Das1, Monoranjan Guchait2, and D. P. Roy3

  • 1Institute of Physics, Sachivalaya Marg, Bhubaneswar 751 005, Orissa, India
  • 2Department of High Energy Physics, Tata Institute of Fundamental Research, 1, Homi Bhabha Road, Mumbai 400 005, India
  • 3Homi Bhabha’s Centre for Science Education, Tata Institute of Fundamental Research, V. N. Purav Marg, Mumbai 400088, India

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Vol. 90, Iss. 5 — 1 September 2014

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