ArticleOriginal scientific text
Title
Technicalities in the calculation of the 3rd post-Newtonian dynamics
Authors 1
Affiliations
- Max-Planck-Society, Research Unit "Theory of Gravitation" at the Friedrich-Schiller-University, 07743 Jena, Germany
Abstract
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.
Bibliography
- R. Arnowitt, S. Deser, and C. W. Misner, The dynamics of general relativity, in: Gravitation: an introduction to current research, L. Witten (ed.), Wiley, New York, 1962, 227-265.
- I. M. Gel'fand and G. E. Shilov, Generalized functions, Academic Press, New York, 1964.
- P. Jaranowski and G. Schäfer, Radiative 3.5 post-Newtonian ADM Hamiltonian for many-body point-mass systems, Phys. Rev. D (1996), submitted.
- P. Jaranowski and G. Schäfer, 3rd post-Newtonian ADM Hamiltonian for two-body point-mass systems, in preparation.
- S. M. Kopeikin, General-relativistic equations of binary motion for extended bodies with conservative corrections and radiation damping, Sov. Astron. 29 (1985), 516-524.
- T. Ohta, H. Okamura, T. Kimura, and K. Hiida, Higher order gravitational potential for many-body system, Progr. Theor. Phys. 51 (1974), 1220-1238.
- M. Riesz, L'intégrale de Riemann-Liouville et le problème de Cauchy, Acta Mathematica 81 (1949), 1-223.
- G. Schäfer, The gravitational quadrupole radiation-reaction force and the canonical formalism of ADM, Annals of Physics 161 (1985), 81-100.