On the structure of the post-Newtonian expansion in general relativity
arXiv:gr-qc/0503075 · doi:10.1103/PhysRevD.72.044024
Abstract
In the continuation of a preceding work, we derive a new expression for the metric in the near zone of an isolated matter system in post-Newtonian approximations of general relativity. The post-Newtonian metric, a solution of the field equations in harmonic coordinates, is formally valid up to any order, and is cast in the form of a particular solution of the wave equation, plus a specific homogeneous solution which ensures the asymptotic matching to the multipolar expansion of the gravitational field in the exterior of the system. The new form provides some insights on the structure of the post-Newtonian expansion in general relativity and the gravitational radiation reaction terms therein.
arXiv comment22 pages, to appear in Phys. Rev. D
References in corpus (7)
- Post-Newtonian gravitational radiation and equations of motion via direct integration of the relaxed Einstein equations. II. Two-body equations of motion to second post-Newtonian order, and radiation-reaction to 3.5 post-Newtonian order
- Second-post-Newtonian generation of gravitational radiation
- On the multipole expansion of the gravitational field
- Gravitational radiation reaction in the equations of motion of compact binaries to 3.5 post-Newtonian order
- The binary black-hole dynamics at the third-and-a-half post-Newtonian order in the ADM-formalism
- Post-Newtonian approximation for isolated systems calculated by matched asymptotic expansions
- Gravitational radiation reaction and balance equations to post-Newtonian order
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