Dynamic dark matter substructure in Milky Way-like halos enhances neutron star dark matter accretion by at most a factor of about two, so it cannot explain the twelve-order-of-magnitude gap between equation-of-state and accretion estimates.
Choudhury et al., A NICER View of the Nearest and Brightest Millisecond Pulsar: PS R J0437–4715, Astrophys
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Evolution of Neutron Star Environment in the Galactic Halo : Implications for Dark Matter Accretion
Dynamic dark matter substructure in Milky Way-like halos enhances neutron star dark matter accretion by at most a factor of about two, so it cannot explain the twelve-order-of-magnitude gap between equation-of-state and accretion estimates.