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In the description of the relativistic two-body interaction, together with the effects of energy and angular momentum losses due to the emission of gravitational radiation, one has to take into account also the loss of linear momentum, which is responsible for the recoil of the center-of-mass of the system.
1901
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1995
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L. Blanchet, “On the multipole expansion of the gravitational field,” Class. Quant. Grav. 15
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M. Favata, S. A. Hughes and D. E. Holz, “How black holes get their kicks: Gravitational radiation recoil revisited,” Astrophys. J. Lett. 607
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2004
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L. Blanchet, M. S. S. Qusailah and C. M. Will, “Gravitational recoil of inspiralling black-hole binaries to second post-Newtonian order,” Astrophys. J. 635
2005
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L. Blanchet, “Gravitational wave tails of tails,” Class. Quant. Grav. 15
2005
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T. Damour and A. Gopakumar, “Gravitational recoil during binary black hole coalescence using the effective one body approach,” Phys. Rev. D 73
2006
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2006
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J. A. Gonzalez, U. Sperhake, B. Bruegmann, M. Hannam and S. Husa, “Total recoil: The Maximum kick from nonspinning black-hole binary inspiral,” Phys. Rev. Lett. 98
2007
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2007
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2013
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