Minimal no-radiation approximation to Einstein's field equations
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[1] P. Diener,et al. Binary black hole initial data for numerical general relativity based on post-Newtonian data , 2002, gr-qc/0207011.
[2] G. Schäfer. Binary Black Holes and Gravitational Wave Production: Post-Newtonian Analytic Treatment , 2003 .
[3] G. B. Cook. Initial Data for Numerical Relativity , 2000, Living reviews in relativity.
[4] T. Damour,et al. Determination of the last stable orbit for circular general relativistic binaries at the third post-Newtonian approximation , 2000, gr-qc/0005034.
[5] R. Price,et al. Nonexistence of conformally flat slices of the Kerr spacetime , 2000, gr-qc/0002013.
[6] G. Schaefer,et al. Relativistic dust disks and the Wilson-Mathews approach , 1998, gr-qc/9812068.
[7] P. Jaranowski,et al. Third post-Newtonian higher order ADM Hamilton dynamics for two-body point-mass systems , 1998 .
[8] Darryl D. Holm. Hamiltonian formalism for general-relativistic adiabatic fluids , 1985 .
[9] G. Schäfer,et al. The gravitational quadrupole radiation-reaction force and the canonical formalism of ADM , 1985 .