\begin{document}$\gtrsim 100$\end{document} GeV per nucleon). If DM particles are heavy, the annihilation productions of DM can be highly boosted, and thus the fluxes of anti-nuclei produced by DM annihilation may exceed the secondary background at high energies, which opens a high energy window for indirect DM detection. We investigate the possibility of detecting heavy DM particles which annihilate into high energy anti-nuclei. We use the Monte Carlo generators PYTHIA, EPOS-LHC and DPMJET and the coalescence model to simulate the production of anti-nuclei, and constrain the DM annihilation cross-sections by using the AMS-02 and HAWC antiproton data and the HESS galactic center \begin{document}$ \gamma $\end{document}-ray data. We find that the conclusion depends on the choice of DM density profiles. For the “Cored” type profile with a DM particle mass \begin{document}$\gtrsim 10$\end{document} TeV, the contributions from DM annihilation can exceed the secondary background in high energy regions, which opens the high energy window, while for the “Cuspy” type profile, the excess disappears."> High energy window for probing dark matter with cosmic-ray antideuterium and antihelium -
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