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Phys. Rev. Lett. 89, 231102 (2002) [4 pages]

Measuring Neutron-Star Radii with Gravitational-Wave Detectors

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Joshua A. Faber, Philippe Grandclément, and Frederic A. Rasio
Department of Physics and Astronomy, Northwestern University, Evanston, Illinois 60208

Keisuke Taniguchi
Department of Earth Science and Astronomy, University of Tokyo, Komaba, Meguro, Tokyo 153-8902, Japan

Received 23 April 2002; published 18 November 2002

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 measurement of the NS masses during inspiral, the determination of M/R will allow very strong constraints to be placed on the equation of state of dense nuclear matter.


©2002 The American Physical Society

URL: http://link.aps.org/doi/10.1103/PhysRevLett.89.231102
DOI: 10.1103/PhysRevLett.89.231102
PACS: 04.30.Db, 47.11.+j, 95.85.Sz, 97.60.Jd

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