A Bayesian analysis of mock neutron star radius measurements shows that precision radii mainly constrain the symmetry-energy parameters L and Ksym and the quark transition density, while transition strength and quark sound speed are encoded in mass-radius topology.
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How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition
A Bayesian analysis of mock neutron star radius measurements shows that precision radii mainly constrain the symmetry-energy parameters L and Ksym and the quark transition density, while transition strength and quark sound speed are encoded in mass-radius topology.