Measuring neutron-star radii with gravitational-wave detectors.

@article{Faber2002MeasuringNR,
  title={Measuring neutron-star radii with gravitational-wave detectors.},
  author={Joshua A. Faber and Philippe Grandcl{\'e}ment and Frederic A. Rasio and Keisuke Taniguchi},
  journal={Physical review letters},
  year={2002},
  volume={89 23},
  pages={
          231102
        }
}
Coalescing binary neutron stars (NS) are expected to be an important source of gravitational waves (GW) detectable by laser interferometers. We present here a simple method for determining the compactness ratio M/R of NS based on the observed deviation of the GW energy spectrum from point-mass behavior at the end of inspiral. Our method is based on the properties of quasiequilibrium binary NS sequences and does not require the computation of the full GW signal h(t). Combined with the… 

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