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arXiv · 0705.3481

Gravitational waveforms for finite mass binaries

Mátyás Vasúth·János Majár
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Abstract

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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Mátyás Vasúth, János Majár. 2007-05-23. Gravitational waveforms for finite mass binaries. https://doi.org/10.1142/s0217751x07036488

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