Post-Newtonian gravitational radiation from orbiting point masses

Details Post-Newtonian gravitational radiation from orbiting point masses Post-Newtonian gravitational radiation from orbiting point masses

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...210..764w&link_type=abstract

Astrophysical Journal, vol. 210, Dec. 15, 1976, pt. 1, p. 764-775.

Astronomy and Astrophysics

Astrophysics

110

Astrophysics, Binary Stars, Gravitational Waves, Point Sources, Relativity, Bremsstrahlung, Circular Orbits, Orbit Calculation, Stellar Luminosity, Two Body Problem

Scientific paper

General formulas are derived which describe the gravitational radiation at large distances from a system of bodies whose sizes are small compared with their separations. The calculation is carried out through post-Newtonian order within general relativity. More explicit formulas are derived for two-body systems, and detailed results are presented for circular orbits, gravitational bremsstrahlung, and head-on collisions.

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