Given the recent constraints from the dark matter (DM) direct detections, we examine a light GeV-scale (2-30 GeV) neutralino DM in the alignment limit of the Minimal Supersymmetric Standard Model (MSSM). In this limit without decoupling, the heavy CP-even scalar plays the role of the Standard Model (SM) Higgs boson while the other scalar can be rather light so that the DM can annihilate through the resonance or into a pair of to achieve the observed relic density. With the current collider and cosmological constraints, we find that such a light neutralino DM above 6 GeV can be excluded by the XENON-1T (2017) limits while the survivied parameter space below 6 GeV can be fully covered by the future germanium-based light dark matter detections (such as CDEX), by the Higgs coupling precison measurements or by the production process at an electron-positron collider (Higgs factory).

生成讲解博客的中文版本

生成AI智能校验的中文版本