A Bayesian analysis of dark matter admixed neutron stars finds that astrophysical data constrain only the dark matter fraction, which is governed by the hadronic equation of state stiffness.
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Exploring Fermionic Dark Matter Admixed Neutron Stars in the Light of Astrophysical Observations
A Bayesian analysis of dark matter admixed neutron stars finds that astrophysical data constrain only the dark matter fraction, which is governed by the hadronic equation of state stiffness.