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Using post-Newtonian equations of motion for fluid bodies valid to the second post-Newtonian order, we derive the equations of motion for binary systems with finite-sized, non-spinning but arbitrarily shaped bodies.
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T. Damour, in 300 Years of Gravitation
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C. M. Will, Theory and Experiment in Gravitational Physics
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M. E. Pati and C. M. Will, Phys. Rev. D 62
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Cited alongside, same era.
L. Blanchet and G. Faye, J. Math. Phys. 42
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Later among the works it cites.
Y. Itoh, T. Futamase, and H. Asada, Phys. Rev. D 63
2001
Later among the works it cites.
M. E. Pati and C. M. Will, Phys. Rev. D 65
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C. M. Will, Phys. Rev. D 71
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C. M. Will, Living Rev. Relativity 9
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H. Wang and C. M. Will, Phys. Rev. D 75
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