Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-04-23
Phys.Rev.Lett. 89 (2002) 231102
Astronomy and Astrophysics
Astrophysics
Minor revisions and ref. updates, RevTeX4, 6 pages, 2 figures, accepted by Phys. Rev. Lett
Scientific paper
10.1103/PhysRevLett.89.231102
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 an inspiral event. Our method is based on the properties of quasi-equilibrium binary NS sequences and does not require the computation of the full GW signal h(t). Combined with the measurement of the NS masses from the GW signal during inspiral, the determination of M/R will allow very strong constraints to be placed on the equation of state of nuclear matter at high densities.
Faber Joshua A.
Grandclement Philippe
Rasio Frederic A.
Taniguchi Keisuke
No associations
LandOfFree
Measuring Neutron Star Radii with Gravitational Wave Detectors does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Measuring Neutron Star Radii with Gravitational Wave Detectors, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Measuring Neutron Star Radii with Gravitational Wave Detectors will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-546