The evidence for distinguishing two neutron-star equations of state grows as SNR to roughly the 1.8 power, with a prefactor set by tidal-deformability contrast, and this scaling predicted an unseen binary configuration's discrimination threshold within 0.3%.
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How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State?
The evidence for distinguishing two neutron-star equations of state grows as SNR to roughly the 1.8 power, with a prefactor set by tidal-deformability contrast, and this scaling predicted an unseen binary configuration's discrimination threshold within 0.3%.