Back to Volume
Paper: Gravitational Waveforms in the Lense-Thirring Approximation
Volume: 349, Astrophysics of Variable Stars
Page: 289
Authors: Majar, J.
Abstract: 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 1.5PN 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.
Back to Volume