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.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.