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Cosmological Probes of Dark Matter Interactions: The Next Decade

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arxiv 1903.05140 v1 pith:ATFSXZ2X submitted 2019-03-12 astro-ph.CO

classification astro-ph.CO
keywords cosmologicaldarkmatterdecadetheoreticaladvancementsalphaanisotropy
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abstract

Cosmological observations offer unique and robust avenues for probing the fundamental nature of dark matter particles-they broadly test a range of compelling theoretical scenarios, often surpassing or complementing the reach of terrestrial and other experiments. We discuss observational and theoretical advancements that will play a pivotal role in realizing a strong program of cosmological searches for the identity of dark matter in the coming decade. Specifically, we focus on measurements of the cosmic-microwave-background anisotropy and spectral distortions, and tracers of structure (such as the Lyman-$\alpha$ forest, galaxies, and the cosmological 21-cm signal).

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Cited by 3 Pith papers

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

  1. Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure

    astro-ph.CO 2025-02 conditional novelty 6.0 of 10

    BOSS full-shape data do not tighten Planck bounds on velocity-dependent dark matter-baryon scattering, but adding a DES S8 prior yields a greater than 2 sigma preference for a velocity-independent cross section and lo...

  2. Mixed Dark Matter: Limits from the Milky Way Satellite Galaxies

    astro-ph.CO 2026-06 unverdicted novelty 5.0 of 10

    New 95% confidence limits on mixed fuzzy dark matter mass and interacting dark matter cross sections are set using Milky Way satellites for beyond-CDM fractions down to 50%, with power-law weakening of bounds and fore...

  3. Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST

    hep-ph 2025-11 conditional novelty 5.0 of 10

    JWST ultraviolet luminosity function data currently provide the strongest upper limits on velocity-dependent (∝v^{-2}) dark matter–proton scattering for sub-GeV dark matter.

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