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- W3100431181 abstract "A third post-Newtonian (3 PN) equation of motion for two spherical compact stars in a harmonic coordinate has been derived based on the surface integral approach and the strong field point particle limit. The strong field point particle limit enables us to incorporate a notion of a self-gravitating regular star into general relativity. The resulting 3 PN equation of motion is Lorentz invariant, unambiguous, and conserves an energy of the binary orbital motion." @default.
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- W3100431181 date "2004-02-05" @default.
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- W3100431181 title "On the equation of motion of compact binaries in the post-Newtonian approximation" @default.
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- W3100431181 doi "https://doi.org/10.1088/0264-9381/21/5/021" @default.
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