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Spin-Dependent Light Dark Matter Constraints from Mediators

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arxiv 1905.04319 v1 pith:SIRGQ47G submitted 2019-05-10 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords darkmatterlightscatteringspin-dependentbeenlimitsastrophysical
verification ladder T0 review T1 audit T2 compute T3 formal
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A bevy of light dark matter direct detection experiments have been proposed, targeting spin-independent dark matter scattering. In order to be exhaustive, non-standard signatures that have been investigated in the WIMP window including spin-dependent dark matter scattering also need to be looked into in the light dark matter parameter space. In this work, we promote this endeavor by deriving indirect limits on sub-GeV spin-dependent dark matter through terrestrial and astrophysical limits on the forces that mediate this scattering.

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  1. Spin-Dependent Scattering of Sub-GeV Dark Matter: Models and Constraints

    hep-ph 2025-06 conditional novelty 8.0 of 10

    A new calculation of spin-dependent sub-GeV dark matter phonon scattering shows only the light scalar mediator model retains testable parameter space, conditional on the supernova trapping window.

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