Gravitational waves from inspiraling compact binaries: Second post-Newtonian waveforms as search templates II
General Relativity and Quantum Cosmology
2016-08-25 v1
Abstract
We present further evidence that the second post-Newtonian (pN) approximation to the gravitational waves emitted by inspiraling compact binaries is sufficient for the detection of these systems. This is established by comparing the 2-pN wave forms to signals calculated from black hole perturbation theory. Results are presented for different detector noise curves. We also discuss the validity of this type of analysis.
Keywords
Cite
@article{arxiv.gr-qc/9806077,
title = {Gravitational waves from inspiraling compact binaries: Second post-Newtonian waveforms as search templates II},
author = {Serge Droz},
journal= {arXiv preprint arXiv:gr-qc/9806077},
year = {2016}
}
Comments
5 pages, 3 Figures, RevTeX