Gravitational waveforms for finite mass binaries

Details Gravitational waveforms for finite mass binaries Gravitational waveforms for finite mass binaries

2007-05-23

arxiv.org/abs/0705.3481v2

Int.J.Mod.Phys.A22:2405-2414,2007

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

7 pages, to appear in IJMPA; corrected typos

Scientific paper

10.1142/S0217751X07036488

One of the promising sources of gravitational radiation is a binary system composed of compact stars. It is an important question how the rotation of the bodies and the eccentricity of the orbit affect the detectable signal. Here we present a method to evaluate the gravitational wave polarization states for inspiralling compact binaries with comparable mass. We consider eccentric orbits and the spin-orbit contribution in the case of one spinning object up to 1.5 post-Newtonian order. For circular orbits our results are in agreement with existing calculations.

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