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.
Golovko, Results in Physics 44, 106164 (2023)
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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.