Second post-Newtonian motion of compact binaries

Details Second post-Newtonian motion of compact binaries Second post-Newtonian motion of compact binaries

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phla..174..196s&link_type=abstract

Physics Letters A, Volume 174, Issue 3, p. 196-205.

Physics

51

Scientific paper

The second post-Newtonian (2pN) motion of binary systems consisting of two nonrotating compact objects (e.g. neutron stars) is explicitly given in the form of a generalized quasi-Keplerian parametrization. All parameters are expressed as functions of energy and angular momentum. The test-mass limit is discussed. The limit of validity of the first and second post-Newtonian approximation for a test mass in Schwarzschild spacetime is investigated.

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