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Literature Catalog: Compact Binaries: Inspiral: Non-Spinning BH Binary
Also sorted by authorLast updated Feb 10, 2004.
2003
L. Blanchet, T. Damour and G. Esposito-Farese, Dimensional regularization of the third postnewtonian dynamics of point particles in harmonic coordinates, 2003.T. Mora and C. M. Will, A post-newtonian diagnostic of quasi-equilibrium binary configurations of compact objects, 2003.
B. Iyer and L. Blanchet, " Third Post-Newtonian dynamics of compact binaries: equations in the center-of-mass frame," to appear in Classical and Quantum Gravity
2002
L. Blanchet, B.R. Iyer and B. Joguet, `` Gravitational waves from inspiralling compact binaries: Energy flux to third post-Newtonian order,'' Phys. Rev. D 65, 064005 (2002)L. Blanchet, G. Faye, B.R. Iyer and B. Joguet, `` Gravitational-wave inspiral of compact binary systems to 7/2 post-Newtonian order,'' Phys. Rev. D 65, 061501 (2002)
L. Blanchet, `` Innermost circular orbit of binary black holes at the third post-Newtonian approximation,'' Phys. Rev. D 65, 124009 (2002)
A. Gopakumar, B.R. Iyer and S. Iyer, `` Second post-Newtonian gravitational wave polarizations for compact binaries in elliptical orbits," Phys. Rev. D 65, 084011 (2002)
M.E. Pati, C.M. Will, `` Post-Newtonian gravitational radiation and equations of motion via direct integration of the relaxed Einstein equations. 2. Two body equations of motion to second post-Newtonian order, and radiation reaction to 3.5 post-Newtonian order," Phys. Rev. D 65, 104008 (2002)
2001
L.Blanchet and G. Faye, `` Lorentzian regularization and the problem of point-like particles in general relativity,'' J. Math. Phys. 42, 4391 (2001)L. Blanchet and G. Faye, `` General relativistic dynamics of compact binaries at the third post-Newtonian order,'' Phys. Rev. D 63, 062005 (2001)
T. Damour, P. Jaranowski and G. Schaefer, `` Equivalence between the ADM-Hamiltonian and the harmonic-coordinates approaches to the third post-Newtonian dynamics of compact binaries,'' Phys. Rev. D 63, 044021 (2001) [Erratum-ibid. D 66, 029901 (2002)].
T. Damour, P. Jaranowski and G. Schaefer, `` Dimensional regularization of the gravitational interaction of point masses,'' Phys. Lett. B 513, 147 (2001)
V.C. de Andrade, L. Blanchet and G. Faye, `` Third post-Newtonian dynamics of compact binaries: Noetherian conserved quantities and equivalence between the harmonic coordinate and ADM-Hamiltonian formalisms,'' Class. Quant. Grav. 18, 753 (2001)
2000
L. Blanchet and G. Faye, `` Equations of motion of point-particle binaries at the third post-Newtonian order,'' Phys. Lett. A 271, 58 (2000)T. Damour, P. Jaranowski and G. Schaefer, `` Dynamical invariants for general relativistic two-body systems at the third post-Newtonian approximation,'' Phys. Rev. D 62, 044024 (2000)
M.E. Pati and C.M. Will, `` Post-Newtonian gravitational radiation and equations of motion via direct integration of the relaxed Einstein equations. 1. Foundations," Phys. Rev. D 62, 124015 (2000)
1999
P. Jaranowski and G. Schaefer, `` The binary black-hole problem at the third post-Newtonian approximation in the orbital motion: Static part,'' Phys. Rev. D 60, 124003 (1999)
1998
L. Blanchet, `` Gravitational-wave tails of tails,'' Class. Quant. Grav. 15, 113 (1998)P. Jaranowski and G. Schaefer, `` Nonuniqueness of the third post-Newtonian binary point mass dynamics," Phys. Rev. D 57, 5948 (1998)
P. Jaranowski and G. Schaefer, `` 3rd post-Newtonian higher order Hamilton dynamics for two-body point-mass systems,'' Phys. Rev. D 57, 7274 (1998) [Erratum-ibid. D 63, 029902 (2001)].
1997
A. Gopakumar, B.R. Iyer and S. Iyer, `` Second post-Newtonian gravitational radiation reaction for two-body systems: Nonspinning bodies,'' Phys. Rev. D 55, 6030 (1997) [Erratum-ibid. D 57, 6562 (1998)].A. Gopakumar and B.R. Iyer, `` Gravitational waves from inspiraling compact binaries: angular momentum flux, evolution of the orbital elements, and the waveform to the second post-Newtonian order," Phys. Rev. D 56, 7708 (1997)
1996
L. Blanchet, B.R. Iyer, C.M. Will and A.G. Wiseman, `` Gravitational wave forms from inspiralling compact binaries to second-post-Newtonian order,'' Class. Quant. Grav. 13, 575 (1996)L. Blanchet, `` Energy losses by gravitational radiation in inspiralling compact binaries to five halves post-Newtonian order,'' Phys. Rev. D 54, 1417 (1996)
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, 4813 (1996)
1995
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, 3515 (1995)L. Blanchet, T. Damour and B.R. Iyer, `` Gravitational waves from inspiralling compact binaries: Energy loss and waveform to second-post-Newtonian order," Phys. Rev. D 51, 5360 (1995)
L. Blanchet, `` Second-post-Newtonian generation of gravitational radiation," Phys. Rev. D 51, 2559 (1995)
B.R. Iyer and C.M. Will, ``Post-Newtonian Gravitational Radiation Reaction For Two Body Systems: Nonspinning Bodies,'' Phys. Rev. D 52, 6882 (1995).
1993
B.R. Iyer and C.M. Will, ``Post-Newtonian Gravitational Radiation Reaction For Two Body Systems,'' Phys. Rev. Lett. 70, 113 (1993).L.E. Kidder, C.M. Will and A.G. Wiseman, ``Coalescing binary systems of compact objects to (post) 2.5-Newtonian order. III. Transition from inspiral to plunge," Phys. Rev. D 47, 3281 (1993)
1992
L.E. Kidder, C.M. Will and A.G. Wiseman, ``Innermost stable orbits for coalescing binary systems of compact objects," Class. Quantum Grav. 9, L127 (1992).
1990
C.W. Lincoln and C.M. Will, ``Coalescing Binary Systems Of Compact Objects To (Post) 5/2 Newtonian Order: Late Time Evolution And Gravitational Radiation Emission,'' Phys. Rev. D 42, 1123 (1990)
1980s
L. Blanchet and G. Schaefer, "Higher order gravitational radiation losses in binary ststems," Mon. Not. R. astr. Soc. 239, 845 (1989).T. Damour and N. Deruelle, ``General relativistic celestial mechanics of binary systems I. The post-Newtonian motion," Ann. Inst. Henri Poincaré 43, 107 (1985)
T. Damour, ``Gravitational radiation reaction in the binary pulsar and the quadrupole-formula controversy," Phys. Rev. Lett. 51, 1019 (1983).
T. Damour, ``The two-body problem and radiation damping in general-relativity,'' Comptes Rendus Acad. Sci. Ser. II 294, 1355 (1982).
L. Bel, T. Damour, N. Deruelle, J. Ibañez, and J. Martin, ``Poincaré-invariant gravitational-field and equations of motion of 2 point-like objects - The post-linear approximtion of general-relativity,'' Gen. Relativ. Gravit. 13, 963 (1981).
T. Damour and N. Deruelle, ``Generalized lagrangian of two point masses in the post-post-Newtonian approximation of general-relativity,'' Comptes Rendus Acad. Sci. Ser. II 293, 537 (1981).
T. Damour and N. Deruelle, ``Radiation Reaction And Angular Momentum Loss In Small Angle Gravitational Scattering,'' Phys. Lett. A 87, 81 (1981).
K.S. Thorne, ``Multipole expansion of gravitational radiation," Rev. Mod. Phys. 52, 285 (1980).
1900 - 1979
R.V. Wagoner and C.M. Will, ``Postnewtonian Gravitational Radiation From Orbiting Point Masses,'' Astrophys. J. 210, 764 (1976) [Erratum-ibid. 215, 984 (1977)].P.C. Peters, ``Gravitational radiation and the motion of two point masses," Phys. Rev. 136, 1224 (1964).
P.C. Peters and J. Mathews, ``Gravitational radiation from point masses in a Keplerian orbit," Phys. Rev. 131, 435 (1963).
L. Landau and E. Lifshitz, ``The classical theory of fields,'' Chap. 11, (Addison-Wesley, Reading Massachusetts, 1959).
A. Einstein, Sb. Preuss. Akad. Wiss. 688 (1916)
A. Einstein, Sb. Preuss. Akad. Wiss. 154 (1918)