Nearly universal inverse mappings between neutron star radius R1.4 and empirical EOS parameters cause precision-dependent shifts in Bayesian posterior means via nonlinear filtering of the radius distribution.
Pacilio, et al., Phys
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Bayesian analysis of a smooth hadron-quark crossover EOS finds current observations tightly constrain the density dependence of nuclear symmetry energy while leaving highest-density hadronic and quark-matter parameters only weakly constrained.
citing papers explorer
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Universal EOS-Radius Inverse Mappings Govern Precision-Dependent Inference of the Neutron Star Equation of State
Nearly universal inverse mappings between neutron star radius R1.4 and empirical EOS parameters cause precision-dependent shifts in Bayesian posterior means via nonlinear filtering of the radius distribution.
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Bayesian Constraints on the Neutron Star Equation of State with a Smooth Hadron-Quark Crossover
Bayesian analysis of a smooth hadron-quark crossover EOS finds current observations tightly constrain the density dependence of nuclear symmetry energy while leaving highest-density hadronic and quark-matter parameters only weakly constrained.