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- W2000788779 abstract "Abstract The equations of motion of compact binary systems have been derived in the post-Newtonian (PN) approximation of general relativity. The current level of accuracy is 3.5PN order. The conservative part of the equations of motion (neglecting the radiation reaction damping terms) is deducible from a generalized Lagrangian in harmonic coordinates, or equivalently from an ordinary Hamiltonian in ADM coordinates. As an application, we investigate the problem of the dynamical stability of circular binary orbits against gravitational perturbations up to the 3PN order. We find that there is no innermost stable circular orbit or ISCO at the 3PN order for equal masses. To cite this article: L. Blanchet, C. R. Physique 8 (2007)." @default.
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- W2000788779 date "2007-01-01" @default.
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- W2000788779 title "General relativistic dynamics of compact binary systems" @default.
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- W2000788779 doi "https://doi.org/10.1016/j.crhy.2006.11.004" @default.
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