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Tidal interactions have a significant influence on the late dynamics of compact binary systems, which constitute the prime targets of the upcoming network of gravitational-wave detectors.
1915
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1952
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1970
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T. Damour, Gravitational Radiation And The Motion Of Compact Bodies, in Gravitational Radiation
1983
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T. Damour and G. Esposito-Farèse, Testing gravity to second post-Newtonian order: A Field theory approach, Phys. Rev. D
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T. Damour and G. Esposito-Farèse, Gravitational wave versus binary-pulsar tests of strong field gravity, Phys. Rev. D
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A. Buonanno and T. Damour, “Effective one-body approach to general relativistic two-body dynamics,” Phys. Rev. D 59
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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
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T. Damour, “Coalescence of two spinning black holes: an effective one-body approach,” Phys. Rev. D 64
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H. Nakano, N. Sago and M. Sasaki, “Gauge problem in the gravitational self force. 2. First postNewtonian force under Regge-Wheeler gauge,” Phys. Rev. D 68
2003
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W.D. Goldberger and I.Z. Rothstein, An Effective field theory of gravity for extended objects, Phys. Rev. D
2006
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