arXiv:1712.03210·v2·High Energy Astrophysical Phenomena
A Strong Test of the Dark Matter Origin of the 1.4 TeV DAMPE Signal Using IceCube Neutrinos
Yue Zhao🇨🇳 · Ke Fang🇺🇸 · Meng Su🇨🇳 · M. Coleman Miller🇺🇸
Abstract
A tentative excess in the electron spectrum at 1.4 TeV was recently reported by the DArk Matter Particle Explorer (DAMPE). A non-astrophysical scenario in which dark matter particles annihilate or decay in a local clump has been invoked to explain the excess. If annihilation channels in the final states are mediated by left-handed leptons as a component in the doublet, neutrinos with similar energies should have been simultaneously produced. We demonstrate that generic dark matter models can be decisively tested by the existing IceCube data. In case of a non-detection, such models would be excluded at the level by the five-year data for a point-like source and by the ten-year data for an extended source of dark matter particles with left-handed leptons.
Comments: match to the published version