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The Effective One-Body formalism of the gravitational two-body problem in general relativity is reconsidered in the light of recent scattering amplitude calculations.
1901
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1906
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1908
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G. Kälin and R. A. Porto, “From Boundary Data to Bound States,” JHEP 01
1910
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1910
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1911
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T. Damour, “Classical and quantum scattering in post-Minkowskian gravity,” Phys. Rev. D 102
1912
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1972
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A. Buonanno and T. Damour, “Effective One-Body Approach to General Relativistic Two-Body Dynamics,” Phys. Rev. D 59
1999
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A. Buonanno and T. Damour, “Transition from Inspiral to Plunge in Binary Black Hole Coalescences,” Phys. Rev. D 62
2000
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T. Damour, P. Jaranowski and G. Schaefer, “On the Determination of the Last Stable Orbit for Circular General Relativistic Binaries at the Third Postnewtonian Approximation,” 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
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P. Jaranowski and G. Schaefer, “Third Postnewtonian Higher Order Adm Hamilton Dynamics for Two-Body Point Mass Systems,” Phys. Rev. D 57
2001
Cited alongside, same era.
2003
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2005
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A. Buonanno, Y. Chen and T. Damour, “Transition from Inspiral to Plunge in Precessing Binaries of Spinning Black Holes,” Phys. Rev. D 74
2018
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2019
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2019
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2021
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2006
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2008
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2010
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T. Damour, “Gravitational scattering, Post-Minkowskian approximation and Effective One-Body theory,” Phys. Rev. D 94
2016
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2018
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2018
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2018
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2021
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2021
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2021
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2021
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2021
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