Sparticle spectroscopy and dark matter in a U(1) B−L extension of MSSM

Autor: Waqas Ahmed, Shabbar Raza, Qaisar Shafi, Cem Salih Un, Bin Zhu
Jazyk: angličtina
Rok vydání: 2021
Předmět:
Zdroj: Journal of High Energy Physics, Vol 2021, Iss 1, Pp 1-24 (2021)
Druh dokumentu: article
ISSN: 1029-8479
DOI: 10.1007/JHEP01(2021)161
Popis: Abstract We consider a class of SUSY models in which the MSSM gauge group is supplemented with a gauged U(1) B−L symmetry and a global U(1) R symmetry. This extension introduces only electrically neutral states, and the new SUSY partners effectively double the number of states in the neutralino sector that now includes a blino (from B − L) and singlino from a gauge singlet superfield. If the DM density is saturated by a LSP neutralino, the model yields quite a rich phenomenology depending on the DM composition. The LSP relic density constraint provides a lower bound on the stop and gluino masses of about 3 TeV and 4 TeV respectively, which is testable in the near future collider experiments such as HL-LHC. The chargino mass lies between 0.24 TeV and about 2.0 TeV, which can be tested based on the allowed decay channels. We also find m τ ˜ 1 ≳ $$ {m}_{\tilde{\tau}1}\gtrsim $$ 500 GeV, and m e ˜ , m μ ˜ , m v ˜ S , P ≳ $$ {m}_{\tilde{e}},{m}_{\tilde{\mu}},{m}_{{\tilde{v}}^{S,P}}\gtrsim $$ 1 TeV. We identify chargino-neutralino coannihilation processes in the mass region 0.24 TeV ≲ m χ ˜ 1 0 ≈ m χ ˜ 1 ± ≲ $$ \lesssim {m}_{{\tilde{\upchi}}_1^0}\approx {m}_{{\tilde{\upchi}}_1^{\pm }}\lesssim $$ 1.5 TeV, and also coannihilation processes involving stau, selectron, smuon and sneutrinos for masses around 1 TeV. In addition, A 2 resonance solutions are found around 1 TeV, and H 2 and H 3 resonance solutions are also shown around 0.5 TeV and 1 TeV . Some of the A 2 resonance solutions with tan β ≳ 20 may be tested by the A/H → τ + τ − LHC searches.. While the relic density constraint excludes the bino-like DM, it is still possible to realize higgsino, singlino and blino-like DM for various mass scales. We show that all these solutions will be tested in future direct detection experiments such as LUX-Zeplin and Xenon-nT.
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