Dark matter admixture increases the central Ricci, Kretschmann, and Ricci-tensor curvature of quarkyonic neutron stars, while quarkyonic matter stiffens the EOS and reduces curvature.
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Dark Matter Effects on the Curvature of Neutron Stars within the new Quarkyonic Model Coupled with Relativistic Mean Field Theory
Dark matter admixture increases the central Ricci, Kretschmann, and Ricci-tensor curvature of quarkyonic neutron stars, while quarkyonic matter stiffens the EOS and reduces curvature.