Speaker
Kai-Kai Duan
Description
Antiprotons serve as a key target for indirect dark matter detection. Solar modulation significantly influences the search for dark matter through antiproton detection. As antiproton particles penetrate the solar system, they are affected by the heliospheric magnetic field and solar wind, especially those with rigidities below 40 GV. Recently, AMS-02 published results from an 11-year solar cycle study on antiprotons. In this analysis, we examine three methods for solving the Parker equation to systematically investigate the observed excess of antiprotons reported by AMS-02.
Author
Co-authors
Mr
Xiao Wang
Mr
Wen-Hao Li
Dr
Zhi-Hui Xu
(Institute of Modern Physics, Chinese Academy of Sciences)
Yue-Lin Sming Tsai
(Purple Mountain Observatory)
Yi-Zhong Fan
