A limit on warm dark matter from Milky Way satellite halos loses most of its force once non-linear regeneration, stripping, and baryon effects are added, leaving the rotation-curve measurement consistent with the revised estimate.
(2022) Measurement of the Dark Matter Velocity Disper- sion with Dwarf Galaxy Rotation Curves
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Discrepancies Between Limits and Measurements of Warm Dark Matter Properties
A limit on warm dark matter from Milky Way satellite halos loses most of its force once non-linear regeneration, stripping, and baryon effects are added, leaving the rotation-curve measurement consistent with the revised estimate.