Abstract
In this paper, we show that positron data from AMS seem to rule out the explanation of the ARCADE isotropic radio background excess in terms of self-annihilating dark matter. In earlier works it was found that leptonic annihilation channels of light dark matter provide a good fit to the excess due to synchrotron emission of the final state particles. However, limits on the self-annihilation cross section derived from the positron data of AMS now severely constrain light self-annihilating dark matter and cross sections below that of a thermal relic are already tested for leptonic annihilation channels. Combining these two results, we conclude that an explanation of the excess in the radio background in terms of self-annihilating dark matter is excluded.
| Original language | English |
|---|---|
| Article number | 127302 |
| Number of pages | 5 |
| Journal | Physical Review D (Particles, Fields, Gravitation and Cosmology) |
| Volume | 90 |
| Issue number | 12 |
| DOIs | |
| Publication status | Published - 17 Dec 2014 |
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