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General Relativity and Gravitation

, Volume 10, Issue 2, pp 129–148 | Cite as

Orbital equations in the relativistic two-body problem

  • G. O'Brien
Research Articles

Abstract

Synge's approximation method is applied to derive the orbital equations for a binary system consisting of two rotating, spherical, rigid bodies of comparable mass and radius. Approximations are based on the weakness of the field and on the distance between the bodies being considered large by comparison with their radii.

Keywords

Approximation Method Binary System Rigid Body Differential Geometry Comparable Mass 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Plenum Publishing Corporation 1979

Authors and Affiliations

  • G. O'Brien
    • 1
  1. 1.School of Theoretical PhysicsDublin Institute for Advanced StudiesDublin 4

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