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Indirect Detection of WIMP Dark Matter: a compact review

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arxiv 1411.1925 v1 pith:QQOX5I4X submitted 2014-11-07 hep-ph astro-ph.COastro-ph.HEhep-ex

classification hep-phastro-ph.COastro-ph.HEhep-ex
keywords detectionclaimsdarkindirectmatterparticlesreviewaccompanied
verification ladder T0 review T1 audit T2 compute T3 formal
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Indirect detection of dark matter particles, i.e. the detection of annihilation or decay products of Weakly Interacting Massive Particles, has entered a pivotal phase as experiments reach sensitivities that probe the most interesting parameter space. This period is naturally accompanied by claims of detection. In this contribution I discuss and compare different probes (gamma-rays, neutrinos and charged cosmic rays) and review the status and prospects of constraints and recent detection claims.

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Cited by 5 Pith papers

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

  1. Optimisation of amplification and gas mixture for directional Dark Matter searches with the CYGNO/INITIUM project

    physics.ins-det 2025-07 conditional novelty 6.0 of 10

    For a He:CF4 optical TPC, an extra electrode below the last GEM doubles the light yield, and 1.6% SF6 enables negative-ion drift with diffusion as low as 45 µm/√cm.

  2. Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential

    astro-ph.CO 2024-12 conditional novelty 6.0 of 10

    A saturating scalar self-interaction lets dark matter halos form Thomas-Fermi solitons, fuzzy solitons, or transitions between them, with even subdominant interactions seeding fuzzy solitons.

  3. Molecular clouds constraints on sub-GeV DM and asteroid-mass PBHs

    hep-ph 2026-07 conditional novelty 5.0 of 10

    Molecular-cloud ionization yields competitive constraints on sub-GeV dark matter annihilation/decay and on asteroid-mass primordial black holes, particularly for PBHs above 10^16 g.

  4. Minimal Dirac seesaw dark matter

    hep-ph 2024-12 conditional novelty 5.0 of 10

    A Z4-symmetric Dirac seesaw makes the imaginary part of a seesaw scalar a stable dark matter candidate and links its phenomenology to gravitational wave and CMB observables.

  5. $f$-mode oscillations of dark matter admixed quarkyonic neutron star

    astro-ph.HE 2024-12 conditional novelty 5.0 of 10

    Dark matter-admixed quarkyonic neutron stars show f-mode frequencies shifted by up to tens of percent, while universal frequency-density and frequency-compactness relations remain approximately valid.

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