A spinless-binary effective-one-body model built from 4PM scattering data is analytically continued to bound orbits, yields a separated wave equation for the gravitational perturbation, and reproduces SXS numerical-relativity binding energies to better than 0.5% up to ISCO.
Poisson, Gravitational radiation from a particle in circular orbit around a black hole
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Effective one-body theory of spinless binary evolution dynamics
A spinless-binary effective-one-body model built from 4PM scattering data is analytically continued to bound orbits, yields a separated wave equation for the gravitational perturbation, and reproduces SXS numerical-relativity binding energies to better than 0.5% up to ISCO.