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Eccentric motion of spinning compact binaries

Manuel Tessmer*

Gerhard Schäfer

  • Institut für Angewandte Physik, Friedrich–Schiller Universität, Albert-Einstein-Straße 15, 07745 Jena, Germany, European Union

  • Theoretisch–Physikalisches Institut, Friedrich–Schiller–Universität, Max–Wien–Platz 1, 07743 Jena, Germany, European Union

  • *M.Tessmer@uni-jena.de
  • Gerhard.Schaefer@uni-jena.de

Phys. Rev. D 89, 104055 – Published 27 May, 2014

DOI: https://doi.org/10.1103/PhysRevD.89.104055

Abstract

The equations of motion for spinning compact binaries on eccentric orbits are treated perturbatively in powers of a fractional mass-difference ordering parameter. The solution is valid through first order in the mass-difference parameter. A canonical point transformation removes the leading-order terms of the spin-orbit Hamiltonian which induce a wiggling precession of the orbital angular momentum around the conserved total angular momentum, a precession which disappears in the case of equal masses or one single spin. Action-angle variables are applied that make a canonical perturbation theory easily treatable.

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