Published May 3, 2017 | Version v1
Journal article

Resonant slepton production and right sneutrino dark matter in left-right supersymmetry

  • 1. Department of Physics, Concordia University,7141 Sherbrooke St. West, Montreal, Quebec, H4B 1R6 (Canada)
  • 2. Institut Universitaire de France,103 boulevard Saint-Michel, 75005 Paris (France)
  • 3. CNRS, UMR 7589, LPTHE,F-75005 Paris (France)
  • 4. Sorbonne Universités, UPMC University Paris 06, UMR 7589, LPTHE,F-75005 Paris (France)
  • 5. Department of Physics and Helsinki Institute of Physics, University of Helsinki,P.O. Box 64, Gustaf Hällströmin katu 2, FI-00014 University of Helsinki (Finland)
  • 6. Regional Centre for Accelerator-based Particle Physics, Harish-Chandra Research Institute, HBNI,Chhatnag Road, Jhusi, Allahabad 211019 (India)

Description

Right-handed sneutrinos are natural components of left-right symmetric supersymmetric models where the gauge sector is extended to include right-handed weak interactions. Unlike in other models where right-handed sneutrinos are gauge singlets, here the right sneutrino is part of a doublet and could be a dark matter candidate whose annihilation proceeds via gauge interactions. We investigate this possibility, and find that relic density, low-energy observable and direct supersymmetry search constraints can be satisfied when the lightest supersymmetric particle is a right-handed sneutrino. We introduce benchmarks for left-right supersymmetric realizations where either a sneutrino or a neutralino is the lightest superpartner. We then study the LHC signals arising through resonant right-handed slepton production via a WR gauge-boson exchange that lead to final states enriched in leptons, additionally containing a large amount of missing transverse momentum, and featuring a low jet multiplicity. We find that such a resonant production would boost the chances of discovering these weakly interacting supersymmetric particles for a mass range extending beyond 1 TeV already with a luminosity of 100 fb−1. Finally, we compare sneutrino versus neutralino scenarios, and comment on differences with other sneutrino dark matter models.

Availability note (English)

Available from http://dx.doi.org/10.1007/JHEP05(2017)015; Available from http://repo.scoap3.org/record/19985

Additional details

Identifiers

Publishing Information

Journal Title
Journal of High Energy Physics (Online)
Journal Volume
2017
Journal Issue
05
Journal Page Range
p. 15
ISSN
1029-8479

Optional Information

Copyright
Copyright (c) OPEN ACCESS, © The Authors
Notes
PUBLISHER-ID: JHEP05(2017)015; ARXIV:1702.02112; OAI: oai:repo.scoap3.org:19985
Funding organization
SCOAP3, CERN, Geneva (Switzerland)