The two-body problem in the (truncated) PPN-theory

Details The two-body problem in the (truncated) PPN-theory The two-body problem in the (truncated) PPN-theory

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cemec..40...77s&link_type=abstract

Celestial Mechanics (ISSN 0008-8714), vol. 40, no. 1, 1987, p. 77-85.

Physics

4

Celestial Mechanics, Gravitation Theory, Two Body Problem, Double Cusps, Orbital Elements, Secular Variations

Scientific paper

The Wagoner-Will (1976) and Brumberg (1972) analytical representations are given for the solution of the two-body problem in the truncated PPN theory; the method of osculating elements is also employed. The first approach yields an expression for the post-Newtonian orbit, allowing the time dependence to be obtained in turn. It is found that Brumberg's perturbing function is sufficiently general to cover the present PPN two-body problem.

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