The Equations of Motion for an Astrophysical Binary with Accuracy 1/ c5

Physics

Scientific paper

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Scientific paper

The generalized Hamiltonian equations of motion for a gravitationally
interacting two-body system, resulting from a slow-motion expansion of
Einstein's field equations up to the order 1/ c5, are given
explicitly. The appearing quadrupole radiation reaction force is
different (in form) from the well-known and often used one.

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