Orbital equations in the relativistic two-body problem

Details Orbital equations in the relativistic two-body problem Orbital equations in the relativistic two-body problem

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979gregr..10..129o&link_type=abstract

General Relativity and Gravitation, vol. 10, Feb. 1979, p. 129-148.

Computer Science

12

Equations Of Motion, Orbit Calculation, Rigid Structures, Rotating Bodies, Spheres, Two Body Problem, Angular Momentum, Center Of Gravity, Gravitational Effects, Spin Dynamics

Scientific paper

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.

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