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Astro 2020 Science White Paper: Cosmic-ray Antinuclei as Messengers for Dark Matter

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arxiv 1904.05938 v2 pith:HCYXZGPG submitted 2019-04-11 astro-ph.HE physics.space-ph

classification astro-ph.HEphysics.space-ph
keywords antinucleidarklow-energymattercosmic-rayphysicswillaccumulating
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The origin of dark matter is a driving question of modern physics. Low-energy antideuterons provide a "smoking gun" signature of dark matter annihilation or decay, essentially free of astrophysical background. Low-energy antiprotons are a vital partner for this analysis, and low-energy antihelium could provide further discovery space for new physics. In the coming decade, AMS-02 will continue accumulating the large statistics and systematic understanding necessary for it to probe rare antinuclei signatures, and GAPS, which is the first experiment optimized specifically for low-energy cosmic antinuclei, will begin several Antarctic balloon campaigns. The connection of cosmic-ray antinuclei and dark matter is reviewed and the outlook in light of experimental progress is presented.

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  1. GAPS: Searching for Dark Matter using Antinuclei in Cosmic Rays

    astro-ph.IM 2019-08 conditional novelty 2.0 of 10

    GAPS is a balloon-borne instrument designed to search for low-energy cosmic-ray antinuclei, especially antideuterons, as a dark matter signal; this paper reports its design and construction status.

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