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.
Bergstr ¨om, Non-baryonic dark matter: observational evidence and detection methods, Reports on Progress in Physics 63 (5) (2000) 793
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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.