Tail effects in the third post-Newtonian gravitational wave energy flux of compact binaries in quasi-elliptical orbits

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

32 pages, 10 figures. Minor changes in text throughout. Matches the published version

Scientific paper

10.1103/PhysRevD.77.064034

The far-zone flux of energy contains hereditary (tail) contributions that depend on the entire past history of the source. Using the multipolar post-Minkowskian wave generation formalism, we propose and implement a semi-analytical method in the frequency domain to compute these contributions from the inspiral phase of a binary system of compact objects moving in quasi-elliptical orbits up to 3PN order. The method explicitly uses the quasi-Keplerian representation of elliptical orbits at 1PN order and exploits the doubly periodic nature of the motion to average the 3PN fluxes over the binary's orbit. Together with the instantaneous (non-tail) contributions evaluated in a companion paper, it provides crucial inputs for the construction of ready-to-use templates for compact binaries moving on quasi-elliptic orbits, an interesting class of sources for the ground based gravitational wave detectors such as LIGO and Virgo as well as space based detectors like LISA.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Tail effects in the third post-Newtonian gravitational wave energy flux of compact binaries in quasi-elliptical orbits 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 Tail effects in the third post-Newtonian gravitational wave energy flux of compact binaries in quasi-elliptical orbits, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Tail effects in the third post-Newtonian gravitational wave energy flux of compact binaries in quasi-elliptical orbits will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-437146

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.