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Building upon recent progress in applying on-shell amplitude techniques to classical observables in general relativity, we propose a closed-form formula for the conservative Hamiltonian of a spinning binary system at the 1st post-Minkowskian (1PM) order.
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N. Arkani-Hamed, Y. t. Huang and D. O’Connell, “Kerr black holes as elementary particles,” JHEP 2001
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G. Kälin and R. A. Porto, “From Boundary Data to Bound States,” JHEP 2001
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T. Damour, “Classical and Quantum Scattering in Post-Minkowskian Gravity,” arXiv:1912.02139 [gr-qc]
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I. B. Khriplovich and G. G. Kirilin, “Quantum power correction to the Newton law,” J. Exp. Theor. Phys. 95
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N. E. J. Bjerrum-Bohr, J. F. Donoghue and B. R. Holstein, “Quantum gravitational corrections to the nonrelativistic scattering potential of two masses,” Phys. Rev. D 67
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W. D. Goldberger and I. Z. Rothstein, “An Effective field theory of gravity for extended objects,” Phys. Rev. D 73
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R. A. Porto, “Post-Newtonian corrections to the motion of spinning bodies in NRGR,” Phys. Rev. D 73
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2008
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2015
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2015
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V. Vaidya, “Gravitational Spin Hamiltonians from the S Matrix,” Phys. Rev. D 91
2015
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2016
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2008
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2010
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2011
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2011
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M. Levi, “Binary Dynamics from Spin1-Spin2 Coupling at Fourth Post-Newtonian Order,” Phys. Rev. D 85
2012
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2016
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2016
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2016
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C. H. Shen, “Gravitational Radiation from Color-Kinematics Duality,” JHEP 1811
2018
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N. Afkhami-Jeddi, S. Kundu and A. Tajdini, “A Bound on Massive Higher Spin Particles,” JHEP 1904
2019
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2019
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