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The gravitational radiation-reaction force acting on perfect fluids at 3.5post-Newtonian order is cast into a form which is directly applicable tonumerical simulations. Extensive use is made of metric-coefficient changesinduced by functional coordinate transformations, of the continuity equation,as well as of the equations of motion. We also present an expressionappropriate for numerical simulations of the radiation field causing the workedout reaction force.Comment: 22 pages to appear in Physical Review

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