陳傳仁Chen, Chuan-Ren蕭又澤Knas Xiao2019-09-052017-08-102019-09-052017http://etds.lib.ntnu.edu.tw/cgi-bin/gs32/gsweb.cgi?o=dstdcdr&s=id=%22G060441030S%22.&%22.id.&http://rportal.lib.ntnu.edu.tw:80/handle/20.500.12235/102507無中文摘要The cosmic ray p ̄/p data from 20 to 450 GeV measured by AMS-02 can be interpreted in terms of DM. By using the GALPROP code, the propagation with DM annihilating to anti-protons is calculated based on the conventional model. The b ̄b, uu ̄ and W+W− final states are considered with different DM masses and annihilating cross-section as free parameters. To see the goodness of fit, the chi-squared test will be used. Once the best-fit parameters are found, the possibility of DM can be discussed.Dark matterIndirect searchDark matterIndirect search