Non-parametric EOS construction from crust to pQCD forces a sound-speed peak and softening that realizes a generalized quark-hadron crossover in massive neutron stars.
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Multi-messenger constraints shrink the residual uncertainty in post-merger frequency f_{2,mean} to ~100 Hz for fixed mass and compactness, well below the unconstrained range.
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The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover
Non-parametric EOS construction from crust to pQCD forces a sound-speed peak and softening that realizes a generalized quark-hadron crossover in massive neutron stars.
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Post-Merger Gravitational-Wave Uncertainties of Binary Neutron Stars under Multi-Messenger EOS Constraints
Multi-messenger constraints shrink the residual uncertainty in post-merger frequency f_{2,mean} to ~100 Hz for fixed mass and compactness, well below the unconstrained range.