@citekhatri

Galactic Positron Excess from Selectively Enhanced Dark Matter Annihilation?

, , and . (2019)cite arxiv:1911.03488Comment: 13 pages, 12 figures, 2 Tables, Comments welcome.

Abstract

Precision measurements of the positron flux in cosmic ray have revealed an unexplained bump in the spectrum around $E300\,GeV$, not clearly attributable to known astrophysical processes. We propose annihilation of dark matter of mass $m_= 780\,GeV$ with a late-time cross section $v = 4.6310^-24\,cm^3\,s^-1$ as a possible source. The nonmonotonic dependence of the annihilation rate on dark matter velocity, owing to a selective $p$-wave Sommerfeld enhancement, allows such a large signal from the Milky Way without violating corresponding constraints from dwarf galaxies. We briefly explore other signatures of this scenario, and outline avenues to test it in future experiments.

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Galactic Positron Excess from Selectively Enhanced Dark Matter Annihilation?

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