Right-handed neutrino dark matter in U(1)<sub>X</sub>SSM
Abstract There is strong evidence for the existence of dark matter in a number of current experiments. We study dark matter using the U (1) X SSM obtained from the U (1) X extension of the minimal supersymmetric standard model. In the U (1) X SSM, we use the right-handed neutrino as a dark matter candidate, whose lightest mass eigenstate has cold dark matter features. In this paper, the relic density of right-handed neutrino as dark matter is investigated. For dark matter scattering, both spin-independent and spin-dependent cross sections are studied. In the final numerical results obtained, some parameter spaces can satisfy the constraints of the relic density and dark matter direct detection experiments.
Authors
- Ming-Yue Liu
- Long Ruan
- Song Gao (ORCID: https://orcid.org/0000-0002-0151-6493)
- Shu-Min Zhao (ORCID: https://orcid.org/0000-0003-4920-8809)
- Tai-Fu Feng (ORCID: https://orcid.org/0000-0002-0273-0141)
Institutions
- Chongqing University (CN)
- Hebei University (CN)
Publication Details
- Journal
- Journal of Physics G Nuclear and Particle Physics
- Published
- 2024-11-21
- DOI
- https://doi.org/10.1088/1361-6471/ad95a8
- Primary Topic
- Particle physics theoretical and experimental studies
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- National Natural Science Foundation of China