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Orbital phase in inspiralling compact binaries

General Relativity and Quantum Cosmology 2016-11-15 v2
Authors: Mátyás Vasúth , Balázs Mikóczi , László Á. Gergely
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Abstract

We derive the rate of change of the mean motion up to the second post-Newtonian order for inspiralling compact binaries with spin, mass quadrupole and magnetic dipole moments on eccentric orbits. We give this result in terms of orbital elements. We also present the related orbital phase for circular orbits.

Keywords

post-newtonian formalism for compact binaries planetary dynamics

Cite

@article{arxiv.gr-qc/0703054,
  title  = {Orbital phase in inspiralling compact binaries},
  author = {Mátyás Vasúth and Balázs Mikóczi and László Á. Gergely},
  journal= {arXiv preprint arXiv:gr-qc/0703054},
  year   = {2016}
}

Comments

to appear in the Proceedings of the Eleventh Marcel Grossmann Meeting 2006, World Scientific, Singapore (2007)

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