Generalized true- and eccentric-anomaly parametrizations for the perturbed Kepler motion

Details Generalized true- and eccentric-anomaly parametrizations for the perturbed Kepler motion Generalized true- and eccentric-anomaly parametrizations for the perturbed Kepler motion

2007-01-27

arxiv.org/abs/gr-qc/0701151v1

Proceedings of the Ninth Marcel Grossmann Meeting 2000 on Recent Developments in Theoretical and Experimental General Relativi

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Scientific paper

The true- and eccentric-anomaly parametrizations of the Kepler motion are generalized to quasiperiodic orbits by considering perturbations of the radial part of kinetic energy as a series in the negative powers of the orbital radius. A toolbox of methods for averaging observables in terms of the energy $E$ and angular momentum $L$ is developed. A broad range of systems governed by the generic Brumberg force, as well as recent applications of the theory of gravitational radiation involve integrals over a period of motion. These integrals are evaluated by using the residue theorem. It is shown that the pole of the integrand is located in the origin and that under certain circumstances an additional pole emerges.

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