Gravitational waves from inspiraling binary black holes
General Relativity and Quantum Cosmology
2009-11-07 v2
Abstract
Binary black holes are the most promising candidate sources for the first generation of earth-based interferometric gravitational-wave detectors. We summarize and discuss the state-of-the-art analytic techniques developed during the last years to better describe the late dynamical evolution of binary black holes of comparable masses.
Cite
@article{arxiv.gr-qc/0203030,
title = {Gravitational waves from inspiraling binary black holes},
author = {Alessandra Buonanno},
journal= {arXiv preprint arXiv:gr-qc/0203030},
year = {2009}
}
Comments
References added and updated; few typos corrected