Post-Newtonian gravitational radiation reaction for two-body systems

Details Post-Newtonian gravitational radiation reaction for two-body systems Post-Newtonian gravitational radiation reaction for two-body systems

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phrvl..70..113i&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 70, no. 2, p. 113-116.

Physics

51

Binary Stars, Equations Of Motion, Gravitational Waves, Pulsars, Two Body Problem, Angular Momentum, Laser Interferometry, Quadrupoles, Stellar Orbits

Scientific paper

We study gravitational radiation reaction in the equations of motion for binary systems to post-Newtonian order (O(v/c)-squared) beyond the quadrupole approximation. The method uses post-Newtonian expressions for energy and angular momentum flux to infinity, and an assumption of energy and angular momentum balance. The equations of motion are valid for general binary orbits. We discuss the coordinate-system dependence of the radiation-reaction formula.

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