Optimizing the third-and-a-half post-Newtonian gravitational radiation-reaction force for numerical simulations

Details Optimizing the third-and-a-half post-Newtonian gravitational radiation-reaction force for numerical simulations Optimizing the third-and-a-half post-Newtonian gravitational radiation-reaction force for numerical simulations

2003-05-27

arxiv.org/abs/gr-qc/0305101v1

Phys.Rev.D68:084001,2003

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

22 pages to appear in Physical Review D

Scientific paper

10.1103/PhysRevD.68.084001

The gravitational radiation-reaction force acting on perfect fluids at 3.5 post-Newtonian order is cast into a form which is directly applicable to numerical simulations. Extensive use is made of metric-coefficient changes induced by functional coordinate transformations, of the continuity equation, as well as of the equations of motion. We also present an expression appropriate for numerical simulations of the radiation field causing the worked out reaction force.

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