Gravitational waves from inspiraling compact binaries: Accuracy of the post-Newtonian waveforms

Preprint

12 January 1998

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.gr-qc/9801038

Abstract

The accuracy of the post-Newtonian waveforms, both in standard and Pade form, is determined by computing their matched-filtering overlap integral with a reference waveform obtained from black-hole perturbation theory.

Keywords

NEWTONIAN WAVEFORMS
PERTURBATION THEORY
GRAVITATIONAL WAVES
INSPIRALING COMPACT
MATCHED FILTERING
COMPACT BINARIES
POST NEWTONIAN
BLACK HOLE

All Related Versions

Version 1, 1998-01-12, ArXiv