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

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dc.creatorFaye, Guillaume
dc.creatorSchaefer, Gerhard
dc.date2003-05-27
dc.date.accessioned2026-07-07T11:46:20Z
dc.date.available2026-07-07T11:46:20Z
dc.descriptionThe 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.
dc.description22 pages to appear in Physical Review D
dc.identifierhttps://arxiv.org/abs/gr-qc/0305101
dc.identifierhttp://arxiv.org/abs/gr-qc/0305101
dc.identifierPhys.Rev.D68:084001,2003
dc.identifierdoi:10.1103/PhysRevD.68.084001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202190
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOptimizing the third-and-a-half post-Newtonian gravitational radiation-reaction force for numerical simulations
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