G. A. Schott, Phil. Mag. 29
1915
Earlier work this paper cites.
Y. Pan et al
Original
1964
Earlier work this paper cites.
E. Brezin, C. Itzykson and J. Zinn-Justin, Relativistic balmer formula including recoil effects, Phys. Rev. D 1
1970
Earlier work this paper cites.
M. Davis, R. Ruffini and J. Tiomno, Pulses of gravitational radiation of a particle falling radially into a Schwarzschild black hole, Phys. Rev. D 5
1972
Earlier work this paper cites.
T. Damour and N. Deruelle, Radiation Reaction And Angular Momentum Loss In Small Angle Gravitational Scattering, Phys. Lett. A 87
1981
Earlier work this paper cites.
T. Damour, Gravitational Radiation And The Motion Of Compact Bodies,, in Gravitational Radiation
1983
Earlier work this paper cites.
G. Schäfer, The gravitational quadrupole radiation reaction force and the canonical formalism of ADM, Annals Phys. 161
1985
Earlier work this paper cites.
S. M. Kopejkin: Astron. Zh. 62
1985
Earlier work this paper cites.
L. Blanchet and T. Damour, Radiative gravitational fields in general relativity I. General structure of the field outside the source, Phil. Trans. Roy. Soc. Lond. A 320
1986
Earlier work this paper cites.
T. Damour and G. Schäfer, Higher order relativistic periastron advances and binary pulsars, Nuovo Cim. B 101
1988
Earlier work this paper cites.
L. Blanchet and T. Damour, Postnewtonian generation of gravitational waves, Annales Poincare Phys. Theor. 50
1989
Earlier work this paper cites.
T. Damour and B. R. Iyer, Multipole analysis for electromagnetism and linearized gravity with irreducible cartesian tensors, Phys. Rev. D 43
1991
Earlier work this paper cites.
T. Damour and B. R. Iyer, PostNewtonian generation of gravitational waves. 2. The Spin moments, Annales Poincare Phys. Theor. 54
1991
Earlier work this paper cites.
L. Blanchet and T. Damour, Hereditary Effects In Gravitational Radiation, Phys. Rev. D 46
1992
Earlier work this paper cites.
A. G. Wiseman, Coalescing Binary Systems Of Compact Objects To (Post)Newtonian5/2 Order.4v: The Gravitational Wave Tail, Phys. Rev. D 48
1993
Earlier work this paper cites.
L. Blanchet and G. Schä fer, Gravitational wave tails and binary star systems, Class. Quant. Grav. 10
1993
Earlier work this paper cites.
C. Cutler, E. Poisson, G. J. Sussman and L. S. Finn, Gravitational radiation from a particle in circular orbit around a black hole. 2: Numerical results for the nonrotating case, Phys. Rev. D 47
1993
Earlier work this paper cites.
R. H. Price and J. Pullin, Colliding black holes: The Close limit, Phys. Rev. Lett. 72
1994
Earlier work this paper cites.
H. Tagoshi and M. Sasaki, PostNewtonian expansion of gravitational waves from a particle in circular orbit around a Schwarzschild black hole, Prog. Theor. Phys. 92
1994
Earlier work this paper cites.
H. Tagoshi and M. Sasaki, PostNewtonian expansion of gravitational waves from a particle in circular orbit around a Schwarzschild black hole, Prog. Theor. Phys. 92
1994
Earlier work this paper cites.
L. Blanchet, Second Postnewtonian Generation Of Gravitational Radiation, Phys. Rev. D 51
1995
Earlier work this paper cites.
L. Blanchet, T. Damour, B. R. Iyer, C. M. Will and A. G. Wiseman, Gravitational Radiation Damping Of Compact Binary Systems To Second Postnewtonian Order, Phys. Rev. Lett. 74
1995
Earlier work this paper cites.
C. M. Will and A. G. Wiseman, Gravitational radiation from compact binary systems: gravitational waveforms and energy loss to second post-Newtonian order, Phys. Rev. D 54
1996
Earlier work this paper cites.
L. Blanchet, T. Damour and B. R. Iyer, Gravitational Waves From Inspiralling Compact Binaries: Energy Loss And Wave Form To Second Postnewtonian Order, Phys. Rev. D 51
1996
Earlier work this paper cites.
T. Tanaka, H. Tagoshi and M. Sasaki, Gravitational waves by a particle in circular orbits around a Schwarzschild black hole: 5.5 post-Newtonian formula, Prog. Theor. Phys. 96
1996
Earlier work this paper cites.
T. Tanaka, H. Tagoshi and M. Sasaki, Prog. Theor. Phys. 96
1996
Earlier work this paper cites.
E. Poisson, Gravitational radiation from a particle in circular orbit around a black hole. 6. Accuracy of the postNewtonian expansion, Phys. Rev. D 52
1997
Earlier work this paper cites.
T. Damour, B. R. Iyer and B. S. Sathyaprakash, Improved filters for gravitational waves from inspiralling compact binaries, Phys. Rev. D 57
1998
Earlier work this paper cites.
L. Blanchet, Quadrupole-quadrupole gravitational waves, Class. Quant. Grav. 15
1998
Earlier work this paper cites.
A. Buonanno and T. Damour, Effective one-body approach to general relativistic two-body dynamics, Phys. Rev. D 59
1999
Earlier work this paper cites.
C. M. Will, Generation of post-Newtonian gravitational radiation via direct integration of the relaxed Einstein equations, Prog. Theor. Phys. Suppl. 136
1999
Earlier work this paper cites.
A. Buonanno and T. Damour, Transition from inspiral to plunge in binary black hole coalescences, Phys. Rev. D 62
2000
Earlier work this paper cites.
T. Damour, P. Jaranowski and G. Schäfer, On the determination of the last stable orbit for circular general relativistic binaries at the third post-Newtonian approximation, Phys. Rev. D 62
2000
Earlier work this paper cites.
M. E. Pati and C. M. Will, Post-Newtonian gravitational radiation and equations of motion via direct integration of the relaxed Einstein equations. I: Foundations, Phys. Rev. D 62
2000
Earlier work this paper cites.
T. Damour, Coalescence of two spinning black holes: An effective one-body approach, Phys. Rev. D 64
2001
Earlier work this paper cites.