For circular equatorial orbits, EOB and MPD dynamics and gravitational-wave fluxes agree for Schwarzschild primaries, while for Kerr the difference grows with spin and is largest for high positive primary spin.
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Comparing effective-one-body and Mathisson-Papapetrou-Dixon results for a spinning test particle on circular equatorial orbits around a Kerr black hole
For circular equatorial orbits, EOB and MPD dynamics and gravitational-wave fluxes agree for Schwarzschild primaries, while for Kerr the difference grows with spin and is largest for high positive primary spin.