Capture-driven accumulation of asymmetric dark matter in neutron stars stays gravitationally subdominant over a Hubble time and produces no detectable changes in tidal observables.
It is therefore important to verify that the captured DM indeed enters the degenerate regime under the astrophys- ical conditions considered here
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Capture Driven Evolution of Asymmetric Dark Matter in Non-rotating Neutron Stars
Capture-driven accumulation of asymmetric dark matter in neutron stars stays gravitationally subdominant over a Hubble time and produces no detectable changes in tidal observables.