Post-Newtonian corrections to the motion of spinning bodies in nonrelativistic general relativity

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Non-relativistic gravitation: from Newton to Einstein and back (2007, methodology): “For a spinning object the lowest order interaction, found in [ 18 ] and translated to”
Les Houches lectures on effective field theories and gravitational radiation (2007, background): “Actually, this is not completely true, as realistic black holes usually hav e non-zero spin, and the inclusion of spin tends to enhance finite size effects [ 25 ].”