Compact binaries inspiralling along quasi-circular orbits are the most plausible gravitational wave (GW) sources for the operational, planned and proposed laser interferometers. We provide new class of restricted post-Newtonian accurate GW templates for non-spinning compact binaries inspiralling along PN accurate quasi-circular orbits. Arguments based on data analysis, theoretical and astrophysical considerations are invoked to show why these time-domain Taylor approximants should be interesting to various GW data analysis communities.
@article{arxiv.0712.3236,
title = {New Class of Gravitational Wave Templates for Inspiralling Compact Binaries},
author = {Achamveedu Gopakumar},
journal= {arXiv preprint arXiv:0712.3236},
year = {2007}
}