  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.
