English

Prospects for Higgs- and Z-resonant Neutralino Dark Matter

High Energy Physics - Phenomenology 2016-03-23 v1 High Energy Physics - Experiment

Abstract

In the minimal supersymmetric standard models, neutralino dark matter with mass of mχmZ/245m_{\chi}\sim m_Z/2\sim 45 GeV and mχmh/262m_{\chi}\sim m_h/2\sim 62 GeV can have the thermal relic abundance Ωχ1h20.120\Omega_{\chi_1}h^2\simeq 0.120 via the ZZ- and Higgs-resonant annihilations, respectively, while avoiding all the current constraints. Phenomenology of such scenarios is determined only by three parameters, Bino mass M1M_1, Higgsino mass μ\mu, and tanβ\tan\beta, in the limit that all other supersymmetric particles and heavy Higgs bosons are decoupled. In this paper, we comprehensively study the constraints and future prospects of the search for such Higgs- and ZZ-resonant neutralino dark matter. It is shown that almost all the parameter space of the scenario will be probed complementarily by the LHC search for the chargino and neutralinos, the direct detection experiments, and the Higgs invisible decay search at the ILC.

Keywords

Cite

@article{arxiv.1510.05378,
  title  = {Prospects for Higgs- and Z-resonant Neutralino Dark Matter},
  author = {Koichi Hamaguchi and Kazuya Ishikawa},
  journal= {arXiv preprint arXiv:1510.05378},
  year   = {2016}
}

Comments

30 pages, 29 figures