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We compute spin-orbit effects in the equations of motion, binding energy and energy loss of binary systems of compact objects at the next-to-leading order in the post-Newtonian (PN) approximation in the effective field theory (EFT) framework.
1903
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C. W. Lincoln and C. M. Will, “Coalescing binary systems of compact objects to ( post ) 5 / 2 {(\mathrm{post})}^{5/2} -Newtonian order: Late-time evolution and gravitational-radiation emission,” Phys. Rev. D
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L. E. Kidder, “Coalescing binary systems of compact objects to ( post ) 5 / 2 (\mathrm{post})^{5/2} -Newtonian order. V. Spin effects,” Phys. Rev. D
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C. M. Will, “Post-Newtonian gravitational radiation and equations of motion via direct integration of the relaxed Einstein equations. III. Radiation reaction for binary systems with spinning bodies,” Phys. Rev. D
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R. A. Porto, “Post-Newtonian corrections to the motion of spinning bodies in NRGR,” Phys. Rev. D
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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
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2010
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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
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R. A. Porto, “The effective field theorist’s approach to gravitational dynamics,” Phys. Rept
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