Dynamics of a point-particle system interacting gravitationally according to the general theory of relativity can be analyzed within the canonical formalism of Arnowitt, Deser, and Misner. To describe the property of being a point particle one can employ Dirac delta distribution in the energy-momentum tensor of the system. We report some mathematical difficulties which arise in deriving the 3rd post-Newtonian Hamilton's function for such a system. We also offer ways to overcome partially these difficulties.
@article{bwmeta1.element.bwnjournal-article-bcpv41z2p55bwm, author = {Jaranowski, Piotr}, title = {Technicalities in the calculation of the 3rd post-Newtonian dynamics}, journal = {Banach Center Publications}, volume = {38}, year = {1997}, pages = {55-63}, zbl = {0891.53063}, language = {en}, url = {http://dml.mathdoc.fr/item/bwmeta1.element.bwnjournal-article-bcpv41z2p55bwm} }
Jaranowski, Piotr. Technicalities in the calculation of the 3rd post-Newtonian dynamics. Banach Center Publications, Tome 38 (1997) pp. 55-63. http://gdmltest.u-ga.fr/item/bwmeta1.element.bwnjournal-article-bcpv41z2p55bwm/
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