Post-Newtonian effects on Lagrange's equilateral triangular solution for the three-body problem
Post-Newtonian equation for the energy levels of a Dirac particle in a static metric
Post-Newtonian expansion for Gauss-Bonnet Gravity
Post-Newtonian Expansion of Gravitational Radiation
Post-Newtonian expansion of gravitational waves from a particle in circular orbit around a Schwarzschild black hole
Post-Newtonian Expansion of Gravitational Waves from a Particle in Circular Orbits around a Rotating Black Hole :Effects of Black Hole Absorption
Post-Newtonian expansion of gravitational waves from a particle in circular orbits around a rotating black hole: Up to $O(v^8)$ beyond the quadrupole formula
Post-Newtonian Expansion of the Ingoing-Wave Regge-Wheeler Function
Post-Newtonian expansions for perfect fluids
Post-Newtonian extension of the Newton-Cartan theory
Post-Newtonian factorized multipolar waveforms for spinning, non-precessing black-hole binaries
Post-Newtonian Frames of Reference
Post-Newtonian Freely Specifiable Initial Data for Binary Black Holes in Numerical Relativity
Post-Newtonian Gravitational Radiation
Post-Newtonian Gravitational Radiation and Equations of Motion via Direct Integration of the Relaxed Einstein Equations. I. Foundations
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
Post-Newtonian gravitational radiation and equations of motion via direct integration of the relaxed Einstein equations. III. Radiation reaction for binary systems with spinning bodies
Post-Newtonian gravitational radiation and equations of motion via direct integration of the relaxed Einstein equations. IV. Radiation reaction for binary systems with spin-spin coupling
Post-Newtonian gravitational radiation and equations of motion via direct integration of the relaxed Einstein equations. V. Evidence for the strong equivalence principle to second post-Newtonian order
Post-Newtonian Hydrodynamic Equations Using the (3+1) Formalism in General Relativity