Second post-Newtonian motion of compact binaries
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[1] T. Damour,et al. Experimental constraints on strong-field relativistic gravity , 1992, Nature.
[2] C. Will,et al. Coalescing binary systems of compact objects to (post)5/2-Newtonian order: Late-time evolution and gravitational-radiation emission. , 1990, Physical review. D, Particles and fields.
[3] J. Weisberg,et al. Further experimental tests of relativistic gravity using the binary pulsar PSR 1913+16 , 1989 .
[4] T. Ohta,et al. The Two-Body Motion and the Periastron Advance in the Post-Post-Newtonian Approximation , 1989 .
[5] T. Ohta,et al. Center of Inertia for the n-Body System in the Post-Post-Newtonian Approximation in General Relativity , 1989 .
[6] T. Ohta,et al. Center of inertia for the post-post-newtonian two-body problem in general relativity , 1988 .
[7] Thibault Damour,et al. Lagrangians forn point masses at the second post-Newtonian approximation of general relativity , 1985 .
[8] T. Damour. GRAVITATIONAL RADIATION REACTION IN THE BINARY PULSAR AND THE QUADRUPOLE FORMULA CONTROVERSY , 1983 .
[9] D. Gal’tsov,et al. RELATIVISTIC CORRECTIONS TO THE GRAVITATIONAL RADIATION OF A BINARY SYSTEM AND THE FINE STRUCTURE OF THE SPECTRUM , 1980 .