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The recently established formalism of a worldline quantum field theory, which describes the classical scattering of massive bodies in Einstein gravity, is generalized up to quadratic order in spin -- for a pair of Kerr black holes revealing a hidden ${\mathcal N}=2$ supersymmetry.
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Ruth Britto, Freddy Cachazo, and Bo Feng, “Generalized unitarity and one-loop amplitudes in N=4 super-Yang-Mills,” Nucl. Phys. B725
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Bence Kocsis, Merse E. Gaspar, and Szabolcs Marka, “Detection rate estimates of gravity-waves emitted during parabolic encounters of stellar black holes in globular clusters,” Astrophys. J. 648
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Rafael A. Porto, “Post-Newtonian corrections to the motion of spinning bodies in NRGR,” Phys. Rev. D 73
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Johan Samsing, “Eccentric Black Hole Mergers Forming in Globular Clusters,” Phys. Rev. D 97
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Chia-Hsien Shen, “Gravitational Radiation from Color-Kinematics Duality,” JHEP 11
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Dimitrios Kosmopoulos and Andres Luna, “Quadratic-in-spin Hamiltonian at 𝒪 \mathcal{O} (G 2
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