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Eccentric motion of spinning compact binaries
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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