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

被引:0
作者
Mariana Frank
Benjamin Fuks
Katri Huitu
Santosh Kumar Rai
Harri Waltari
机构
[1] Concordia University,Department of Physics
[2] Sorbonne Universités,Department of Physics and Helsinki Institute of Physics
[3] UPMC Univ. Paris 06,undefined
[4] UMR 7589,undefined
[5] LPTHE,undefined
[6] CNRS,undefined
[7] UMR 7589,undefined
[8] LPTHE,undefined
[9] Institut Universitaire de France,undefined
[10] University of Helsinki,undefined
[11] Regional Centre for Accelerator-based Particle Physics,undefined
[12] Harish-Chandra Research Institute,undefined
[13] HBNI,undefined
来源
Journal of High Energy Physics | / 2017卷
关键词
Supersymmetry Phenomenology;
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摘要
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.
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