Future 0.1 km precision neutron star radius measurements will tighten constraints on the symmetry energy and hadron-quark transition density, but will not constrain the quark matter sound speed.
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Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii
Future 0.1 km precision neutron star radius measurements will tighten constraints on the symmetry energy and hadron-quark transition density, but will not constrain the quark matter sound speed.