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Reconstructing the neutron-star equation of state with gravitational-wave detectors from a realistic population of inspiralling binary neutron stars
Gravitational-wave observations of inspiralling binary neutron-star systems can be used to measure the neutron-star equation of state (EOS) through the tidally induced shift in the waveform phase that depends on the tidal deformability parameter $\ensuremath{\lambda}$. Previous work has shown that $\ensuremath{\lambda}$, a function of the neutron-star EOS and mass, is …