The three components S, T, W of PPN perturbation for the rotating two-body problem.

Details The three components S, T, W of PPN perturbation for the rotating two-body problem. The three components S, T, W of PPN perturbation for the rotating two-body problem.

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ppmto..10..128h&link_type=abstract

Publ. Purple Mt. Obs., Vol. 10, No. 2, p. 128 - 135

Computer Science

Scientific paper

A PPN equation of motion for the rotating two-body problem is derived.
This equation is then applied to obtain the three components S, T, W of
rotating PPN perturbation for three conditions and the three components
can be integrated. These components are suitable for conspicuous
rotating effects with study of solar system or binary systems.

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