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A novel approach to the Effective One-Body description of gravitationally interacting two-body systems is introduced.
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T. Damour and G. Esposito-Farèse, “Testing gravity to second postNewtonian order: A Field theory approach,” Phys. Rev. D 53
1996
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T. Damour, B. R. Iyer and B. S. Sathyaprakash, “Improved filters for gravitational waves from inspiralling compact binaries,” Phys. Rev. D 57
1998
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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
Cited alongside, same era.
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
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2008
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T. Damour, “Coalescence of two spinning black holes: an effective one-body approach,” Phys. Rev. D 64
2001
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F. Pretorius, “Evolution of binary black hole spacetimes,” Phys. Rev. Lett. 95
2005
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M. Campanelli, C. O. Lousto, P. Marronetti and Y. Zlochower, “Accurate evolutions of orbiting black-hole binaries without excision,” Phys. Rev. Lett. 96
2006
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J. G. Baker, J. Centrella, D. I. Choi, M. Koppitz and J. van Meter, “Gravitational wave extraction from an inspiraling configuration of merging black holes,” Phys. Rev. Lett. 96
2006
Cited alongside, same era.
A. Buonanno, G. B. Cook and F. Pretorius, “Inspiral, merger and ring-down of equal-mass black-hole binaries,” Phys. Rev. D 75
2007
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2007
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2007
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2013
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