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We develop a general formalism for computing classical observables for relativistic scattering of spinning particles, directly from on-shell amplitudes.
1901
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A. Buonanno and T. Damour, Transition from inspiral to plunge in binary black hole coalescences , Phys. Rev. D62
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T. Damour, Coalescence of two spinning black holes: an effective one-body approach , Phys. Rev. D64
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R. A. Porto, Post-Newtonian corrections to the motion of spinning bodies in NRGR , Phys. Rev. D73
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A. Ross and B. R. Holstein, Spin effects in the effective quantum field theory of general relativity , J. Phys. A: Math. Theor. 40
2007
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2009
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2010
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M. Mathisson, Republication of: New mechanics of material systems , Gen. Relativ. Grav. 42
2010
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2011
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M. Levi, Binary dynamics from spin1-spin2 coupling at fourth post-Newtonian order , Phys. Rev. D85
2012
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D. Neill and I. Z. Rothstein, Classical Space-Times from the S Matrix , Nucl. Phys. B877
2013
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2017
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N. Bahjat-Abbas, A. Luna and C. D. White, The Kerr-Schild double copy in curved spacetime , JHEP 12
2017
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W. D. Goldberger and A. K. Ridgway, Bound states and the classical double copy , Phys. Rev. D97
2018
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C.-H. Shen, Gravitational Radiation from Color-Kinematics Duality , JHEP 11
2018
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C. Lorcé, New explicit expressions for Dirac bilinears , Phys. Rev. D97
2018
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