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Towards the fourth post-Newtonian Hamiltonian for two-point-mass systems

Piotr Jaranowski and Gerhard Schäfer
Phys. Rev. D 86, 061503(R) – Published 11 September 2012

Abstract

The article presents the conservative dynamics of gravitationally interacting two-point-mass systems up to the eight order in the inverse power of the velocity of light, i.e., fourth post-Newtonian (4PN) order and up to quadratic order in Newton’s gravitational constant. Additionally, all logarithmic terms at the 4PN order are given as well as terms describing the test-mass limit. With the aid of the Poincaré algebra, additional terms are obtained. The dynamics is presented in the form of an autonomous Hamiltonian derived within the formalism of Arnowitt, Deser, and Misner. Out of the 57 different terms of the 4PN Hamiltonian in the center-of-mass frame, the coefficients of 45 of them are derived. Reduction of the obtained results to circular orbits is performed resulting in the 4PN-accurate formula for energy expressed in terms of angular frequency in which two coefficients are obtained for the first time.

  • Received 30 July 2012

DOI:https://doi.org/10.1103/PhysRevD.86.061503

© 2012 American Physical Society

Authors & Affiliations

Piotr Jaranowski*

  • Faculty of Physics, University of Białystok, Lipowa 41, 15–424 Białystok, Poland

Gerhard Schäfer

  • Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität, Max-Wien-Pl. 1, 07743 Jena, Germany

  • *pio@alpha.uwb.edu.pl
  • gos@tpi.uni-jena.de

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Issue

Vol. 86, Iss. 6 — 15 September 2012

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