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We use effective field theory techniques to compute the potentials due to spin-spin and spin-orbit effects, from which the O (S₁S₂) contribution to the motion of spinning compact binaries to third Post-Newtonian (PN) order follow. We use a formalism which allows us to impose the spin supplementary condition (SSC) in a canonical framework to all orders in the PN expansion. We explicitly show the equivalence with our previous results, obtained using the Newton-Wigner SSC at the level of the action for spin-spin and spin-orbit potentials reported in arXiv: gr-qc/0604099 and arXiv: 0712. 2032, respectively.
Porto et al. (Thu,) studied this question.
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