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Indirect Detection of Dark Matter in the Galaxy

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arxiv 2006.00513 v1 pith:AST2MXZM submitted 2020-05-31 hep-ph astro-ph.HE

classification hep-phastro-ph.HE
keywords darkmatterfutureindirectrayssearchessignalswaves
verification ladder T0 review T1 audit T2 compute T3 formal
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I present a short overview of the latest developments in indirect searches for dark matter using gamma rays, X-rays, charged cosmic rays, micro waves, radio waves, and neutrinos. I briefly outline key past, present, and future experiments and their search strategies. In several searches there are exciting anomalies which could potentially be emerging dark matter signals. I discuss these anomalous signals, and some future prospects to determine their origins.

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Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Search for Dark Matter Annihilation and Decay with H$\alpha$ Line Emission

    hep-ph 2025-12 conditional novelty 7.0 of 10

    H-alpha line emission from recombining gas in quiet dwarf galaxies is a new probe of dark matter annihilation/decay, giving leading limits for some dark matter masses.

  2. Expanding stellar associations as Galactic accelerometers

    astro-ph.GA 2026-08 conditional novelty 6.0 of 10

    Expanding young stellar associations can be used to constrain the Milky Way's gravitational potential by finding the trial potential that minimizes their reconstructed size at birth.

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