Abstract

Highly accurate measurements of cosmic ray electron flux by the dark matter particle explorer (DAMPE) ranging between 25 GeV and 4.6 TeV have recently been published. A sharp peak structure was found at $\rm~\sim~1.4~~TeV$. This unexpected peak structure can be reproduced by the annihilation/decay of a nearby dark matter (DM) halo. In this study, we adopt the decaying-DM model to interpret the $\rm~\sim~1.4~~TeV$ peak. We found that the decay products of the local DM subhalo could contribute to the DMAPE peak with $m_{\rm~DM}=~{\rm~3~}$ TeV and $\tau~\sim~{\rm~10^{28}}$ s. We also obtain constraints on DM lifetime and the distance of the local DM subhalo by comparison with DAMPE data.

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