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How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition
high-energy-astrophysical-phenomenahigh-energy-physics-phenomenologynuclear-experimentnuclear-theory
We investigate how future high-precision neutron star (NS) radius measurements encode microscopic information about the dense-matter equation of state (EOS), focusing on a possible first-order hadron--quark phase transition and the resulting mass--radius topology. Within a Bayesian framework using m
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