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Using a recent, novel Hamiltonian formulation of the gravitational interaction of spinning binaries, we extend the Effective One Body (EOB) description of the dynamics of two spinning black holes to next-to-leading order (NLO) in the spin-orbit interaction.
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2000
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2000
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T. Damour, “Coalescence of two spinning black holes: An effective one-body approach,” Phys. Rev. D 64
2001
Cited alongside, same era.
T. Damour, P. Jaranowski, and G. Schäfer, “Poincaré invariance in the ADM Hamiltonian approach to the general relativistic two-body problem,” Phys. Rev. D 62
2001
Cited alongside, same era.
T. Damour, P. Jaranowski, and G. Schäfer, “Dimensional regularization of the gravitational interaction of point masses,” Phys. Lett. B 513
2001
Cited alongside, same era.
L. Blanchet, “Innermost circular orbit of binary black holes at the third post-Newtonian approximation,” Phys. Rev. D 65
2002
Cited alongside, same era.
A. Buonanno, Y. Chen, and T. Damour, “Transition from inspiral to plunge in precessing binaries of spinning black holes,” Phys. Rev. D 74
2006
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2007
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2007
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L. Blanchet, A. Buonanno, and G. Faye, “Higher-order spin effects in the dynamics of compact binaries. II: Radiation field,” Phys. Rev. D 74
2007
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M. Campanelli, C. O. Lousto, Y. Zlochower, B. Krishnan, and D. Merritt, “Spin flips and precession in black-hole-binary mergers,” Phys. Rev. D 75
2007
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G. Faye, L. Blanchet, and A. Buonanno, “Higher-order spin effects in the dynamics of compact binaries. I: Equations of motion,” Phys. Rev. D 74
2006
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2007
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T. Damour, A. Nagar et al., in preparation
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2007
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2008
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