English

Light neutralino dark matter in $U(1)_X$SSM

High Energy Physics - Phenomenology 2021-07-14 v3

Abstract

The U(1)XU(1)_X extension of the minimal supersymmetric standard model(MSSM) is called as U(1)XU(1)_XSSM with the local gauge group SU(3)C×SU(2)L×U(1)Y×U(1)XSU(3)_C\times SU(2)_L \times U(1)_Y \times U(1)_X. U(1)XU(1)_XSSM has three singlet Higgs superfields beyond MSSM. In U(1)XU(1)_XSSM, the mass matrix of neutralino is 8×88\times8, whose lightest mass eigenstate possesses cold dark matter characteristic. Supposing the lightest neutralino as dark matter candidate, we study the relic density. For dark matter scattering off nucleus, the cross sections including spin-independent and spin-dependent are both researched. In our numerical results, some parameter space can satisfy the constraints from the relic density and the experiments of dark matter direct detection.

Keywords

Cite

@article{arxiv.2008.06209,
  title  = {Light neutralino dark matter in $U(1)_X$SSM},
  author = {Shu-Min Zhao and Guo-Zhu Ning and Jing-Jing Feng and Hai-Bin Zhang and Tai-Fu Feng},
  journal= {arXiv preprint arXiv:2008.06209},
  year   = {2021}
}

Comments

23 pages, 9 figures

R2 v1 2026-06-23T17:51:09.719Z