AM  Vol.2 No.2 , February 2011
Formulation of the Post-Newtonian Equations of Motion of the Restricted Three Body Problem
In the present work the geodesic equation represents the equations of motion of the particles along the geodesics is derived. The deviation of the curved space-time metric tensor from that of the Minkowski tensor is considered as a perturbation. The quantities is expanded in powers of c-2. The equations of motion of the relativistic three body problem in the PN formalism are obtained.

Cite this paper
nullF. Abd El-Salam and S. El-Bar, "Formulation of the Post-Newtonian Equations of Motion of the Restricted Three Body Problem," Applied Mathematics, Vol. 2 No. 2, 2011, pp. 155-164. doi: 10.4236/am.2011.22018.

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