In this section, we give a simple and divergence free derivation of the equations of motion for a small
compact object with mass around any sort of massive body, following the paper by Fukumoto and
co-authors [78]. The object moves along the geodesic determined by the smooth part of the geometry
around the object up to order
. We note that the smooth part includes the gravitational waves emitted
by the orbital motion of the object. Thus it generalizes the equivalence principle for such a compact object
to the emission of gravitational waves. Also our derivation of the equations of motion provides a
useful method to explicitly calculate the radiation reaction in the fast motion of a compact
body.
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