Detection of gravitational waves from inspiraling compact binaries using non-restricted post-Newtonian approximations

Details Detection of gravitational waves from inspiraling compact binaries using non-restricted post-Newtonian approximations Detection of gravitational waves from inspiraling compact binaries using non-restricted post-Newtonian approximations

2000-05-16

arxiv.org/abs/gr-qc/0005058v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Latex, 6 pages. To appear in: "Rencontres de Moriond: Gravitational waves and experimetal gravity". Edt. J. Dumarchez; Edition

Scientific paper

The set up of matched filters for the detection of gravitational waves from in-spiraling compact binaries is usually carried out using the restricted post-Newtonian approximation: the filter phase is modelled including post-Newtonian corrections, whereas the amplitude is retained at the Newtonian order. Here we investigate the effects of the introduction of post-Newtonian corrections also to the amplitude and we discuss some of the implications for signal detection and parameter estimation.

Affiliated with

Also associated with

No associations

Rating

Detection of gravitational waves from inspiraling compact binaries using non-restricted post-Newtonian approximations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Detection of gravitational waves from inspiraling compact binaries using non-restricted post-Newtonian approximations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detection of gravitational waves from inspiraling compact binaries using non-restricted post-Newtonian approximations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-441417