Scalar neutrino dark matter in $U(1)_X$SSM
High Energy Physics - Phenomenology
2020-03-18 v5
Abstract
SSM is the extension of the minimal supersymmetric standard model(MSSM) and its local gauge group is . To obtain this model, three singlet new Higgs superfields and right-handed neutrinos are added to MSSM. In the framework of SSM, we study the Higgs mass and take the lightest CP-even sneutrino as a cold dark matter candidate. For the lightest CP-even sneutrino, the relic density and the cross section for dark matter scattering off nucleon are both researched. In suitable parameter space of the model, the numerical results satisfy the constraints of the relic density and the cross section with the nucleon.
Cite
@article{arxiv.1905.11007,
title = {Scalar neutrino dark matter in $U(1)_X$SSM},
author = {Shu-Min Zhao and Tai-Fu Feng and Ming-Jie Zhang and Jin-Lei Yang and Hai-Bin Zhang and Guo-Zhu Ning},
journal= {arXiv preprint arXiv:1905.11007},
year = {2020}
}
Comments
28 pages, 6 figures