Evolution of circular, nonequatorial orbits of Kerr black holes due to gravitational-wave emission. II. Inspiral trajectories and gravitational waveforms

Scott A. Hughes(Kavli Institute for Particle Astrophysics and Cosmology)
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields
August 24, 2001
Cited by 229


Related Papers

Using Gravitational‐Wave Standard Sirens
|The Astrophysical Journal|2005|784
Measuring gravitational waves from binary black hole coalescences. I. Signal to noise for inspiral, merger, and ringdown
|Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields|1998|619
Consequences of Gravitational Radiation Recoil
|The Astrophysical Journal|2004|381
The basics of gravitational wave theory
|New Journal of Physics|2005|363