Dark matter admixed quarkyonic stars in a two-fluid model can reproduce the GW190814 secondary mass with either DM cores or DM halos, but the candidate configurations are selected by tuning free parameters.
Kouvaris, Wimp annihilation and cooling of neutron stars, Phys
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Core or Halo? Two-Fluid Analysis of Dark Matter-Admixed Quarkyonic Stars in the Multi-Messenger Era
Dark matter admixed quarkyonic stars in a two-fluid model can reproduce the GW190814 secondary mass with either DM cores or DM halos, but the candidate configurations are selected by tuning free parameters.