A new definition for parameterizing perturbed Kepler dynamics

Physics

Scientific paper

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Scientific paper

Event rate estimations show that parabolic and hyperbolic encounters of compact objects will become significant sources for advanced ground-based gravitational wave detectors. To analytically describe the motion of the objects and the emitted gravitational waveforms a suitable parameterization is needed to be introduced. In the following paper such a parameterization is defined which is valid for both bound and open orbits. First post-Newtonian and spin-orbit corrections are described in detail.

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