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We compute the conservative two-body Hamiltonian of a compact binary system with a spinning black hole through $\mathcal{O}(G^3)$ to all orders in velocity, including linear and quadratic spin terms.
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Guillaume Faye, Luc Blanchet, and Alessandra Buonanno, “Higher-order spin effects in the dynamics of compact binaries. I. Equations of motion,” Phys. Rev. D 74
2006
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Rafael A. Porto, “Post-Newtonian corrections to the motion of spinning bodies in NRGR,” Phys. Rev. D 73
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Rafael A. Porto and Ira Z. Rothstein, “The Hyperfine Einstein-Infeld-Hoffmann potential,” Phys. Rev. Lett. 97
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