Gravitational Waveforms in the Lense-Thirring Approximation

Details Gravitational Waveforms in the Lense-Thirring Approximation Gravitational Waveforms in the Lense-Thirring Approximation

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..349..289m&link_type=abstract

Astrophysics of Variable Stars, Pecs, Hungary, 5-10 September 2005, Sterken, C. and Aerts, C. (eds). ASP Conference Series, Vol.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present the method of determining the detectable gravitational waveform of a binary system. This waveform is expressed with the use of the post-Newtonian (PN) approximation up to 1.5 PN order. Beyond point mass effects we investigate the influence of the rotation of the bodies on the waveform to linear order, in the case of eccentric orbits. The motion is described in the Lense-Thirring picture, where a non-rotating test particle orbits around a slowly rotating compact object.

Affiliated with

Also associated with

No associations

Rating

Gravitational Waveforms in the Lense-Thirring Approximation 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 Gravitational Waveforms in the Lense-Thirring Approximation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gravitational Waveforms in the Lense-Thirring Approximation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1160683