Abstract
Contemporarily, the detection of dark matter is still an unsolved issue for modern physics. Among all the candidates of the dark matter models, the axion and Weakly interacting massive particles (WIMPs) are the most two appealing cases for realizing detection. On this basis, this paper investigates the analytical model construction of the axion and WIMPs based on the concepts of standard model. Subsequently, the detection mechanisms as well as the state-of-art facilities are demonstrated, respectively. Eventually, guideline for future detection and improvement scheme are proposed in order to find the dark matter mass region. Overall, these results shed light on future dark matter detection and model construction.
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