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.
III A 1, we construct a se- quence of equilibrium two fluid TOV solutions parame- terized by the central Fermi momentumk F,c
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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.