Power-law correlations between fractional-maximum-mass radii and central EOS quantities provide a new, fast inversion of neutron star mass-radius curves into the dense-matter equation of state.
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Correlations between the Neutron Star Mass-Radius Relation and the Equation of State of Dense Matter
Power-law correlations between fractional-maximum-mass radii and central EOS quantities provide a new, fast inversion of neutron star mass-radius curves into the dense-matter equation of state.