Third POST Newtonian Equation of Motion for Relativistic Compact Binaries

Details Third POST Newtonian Equation of Motion for Relativistic Compact Binaries Third POST Newtonian Equation of Motion for Relativistic Compact Binaries

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1364i&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

We derive a third post-Newtonian equation of motion for two self-gravitating point masses in a harmonic coordinate using surface integral approach and strong field point particle limit. Our equation of motion is unambiguous, Lorentz invariant (in the post-Newtonian perturbative sense), and conservative (modulo the radiation reaction effect). Namely, we determine the ambiguous parameter found by the other works.

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