Post-Newtonian effects in the motion of two bodies with comparable masses

Details Post-Newtonian effects in the motion of two bodies with comparable masses Post-Newtonian effects in the motion of two bodies with comparable masses

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mvsfa..31...22d&link_type=abstract

Moskovskii Universitet, Vestnik, Seriia 3 - Fizika, Astronomiia (ISSN 0579-9392), vol. 31, Mar.-Apr. 1990, p. 22-27. In Russian.

Astronomy and Astrophysics

Astronomy

Euler-Lagrange Equation, Gravitational Effects, Planetary Orbits, Pulsars, Space-Time Functions, Algorithms, Gravitational Fields, Orbital Mechanics, Two Body Problem

Scientific paper

The motion of systems consisting of two self-gravitating bodies with comparable masses is examined in the framework of an expanded variant of the parameterized post-Newtonian formalism. It is shown that the dynamical characteristics of the two bodies in motion depend significantly on the post-Newtonian parameter theta. A method for determining this parameter from data obtained in a study of the PSR1913+16 pulsor system is discussed.

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