Elliptic waveforms for inspiralling compact binaries

Details Elliptic waveforms for inspiralling compact binaries Elliptic waveforms for inspiralling compact binaries

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010jphcs.218a2011m&link_type=abstract

Journal of Physics: Conference Series, Volume 218, Issue 1, pp. 012011 (2010).

Physics

Scientific paper

The inspiral of supermassive black hole binary systems with high orbital eccentricity are the most promising sources for the gravitational wave observatories. The importance of elliptic gravitational waveforms in various physical scenarios has been emphasized by several authors (Wahlquist 1987, Moreno-Garrido, Buitrago and Mediavilla 1994, Martel and Poisson 1999). Taking into account the eccentricity of the orbit in the total waveform improves the parameter estimation for these sources, as it is shown by the construction and analyzation of the Fisher information matrix. In our work we use the Fourier-Bessel analysis of the Kepler motion and the stationary phase approximation of time-depend waveforms.

Affiliated with

Also associated with

No associations

Rating

Elliptic waveforms for inspiralling compact binaries 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 Elliptic waveforms for inspiralling compact binaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Elliptic waveforms for inspiralling compact binaries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-884303