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Solar Gamma Ray Constraints on Dark Matter Annihilation to Secluded Mediators

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arxiv 2103.16794 v2 pith:NCL2WWCY submitted 2021-03-31 hep-ph astro-ph.HEastro-ph.SR

classification hep-phastro-ph.HEastro-ph.SR
keywords darkmattergammamediatorsconstraintssolarannihilatesconsider
verification ladder T0 review T1 audit T2 compute T3 formal

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We consider the indirect detection of dark matter that is captured in the Sun and subsequently annihilates to long-lived dark mediators. If these mediators escape the Sun before decaying, they can produce striking gamma ray signals, either via the decay of the mediators directly to photons, or via bremsstrahlung and hadronization of the mediator decay products. Using recent measurements from the HAWC Observatory, we determine model-independent limits on heavy dark matter that are orders of magnitude more powerful than direct detection experiments, for both spin-dependent and spin-independent scattering. We also consider a well-motivated model in which fermionic dark matter annihilates to dark photons. For such a realistic scenario, the strength of the solar gamma ray constraints are reduced, compared to the idealistic case, because the dark matter capture cross section and mediator lifetime are related. Nonetheless, solar gamma ray constraints enable us to exclude a previously unconstrained region of dark photon parameter space.

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Cited by 4 Pith papers

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

  1. Complementary Planetary Spectroscopy Probes of Dark Matter

    hep-ph 2025-08 conditional novelty 6.0 of 10

    Dark matter annihilation energy deposited in planetary atmospheres and interiors, compared against existing UV airglow and heat flow measurements, yields new sub-GeV scattering constraints and long-lived mediator reach.

  2. Can a Dark Inferno Melt Earth's Core?

    hep-ph 2025-05 conditional novelty 6.0 of 10

    Dark matter annihilation inside Earth would melt a substantial fraction of the inner core for cross sections previously allowed by surface heat-flow limits.

  3. Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry

    hep-ph 2024-12 conditional novelty 6.0 of 10

    An anomaly-free two-component secluded WIMP model with a dark photon, dark Higgs, and scotogenic Dirac neutrino masses can account for the observed relic density while evading cosmological bounds.

  4. Searching for dark matter annihilating into light long-lived mediators from stars inside dwarf spheroidal galaxies

    astro-ph.HE 2025-01 conditional novelty 5.0 of 10

    Fermi-LAT observations of ten dwarf spheroidals place upper limits on dark matter-nucleon scattering by modeling stellar capture and annihilation through long-lived mediators.

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