The importance of gravitational self-field effects in binary systems with compact objects. II. The ``static two-body problem'' and the attraction law in a post-post-Newtonian approximation of general relativity

Details The importance of gravitational self-field effects in binary systems with compact objects. II. The ``static two-body problem'' and the attraction law in a post-post-Newtonian approximation of general relativity The importance of gravitational self-field effects in binary systems with compact objects. II. The ``static two-body problem'' and the attraction law in a post-post-Newtonian approximation of general relativity

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978gregr...9..821r&link_type=abstract

General Relativity and Gravitation, Volume 9, Issue 9, pp.821-833

Computer Science

2

Binaries:Compact Objects

Scientific paper

The attraction force of two massive bodies connected by a rod is calculated in a post-post-Newtonian approximation. As far as we know this is the first calculation in such an order of approximation. Although the result already shows a complicated field-field interaction, we reproduce Newton's attraction forceM 1 M 2/R 2 as the leading term in powers of 1/R.

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