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Gravitational self-force theory is the leading approach for modeling gravitational wave emission from small mass-ratio compact binaries.
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J. Thornburg and B. Wardell, Scalar self-force for highly eccentric equatorial orbits in kerr spacetime, Physical Review D 95
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2019
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S.-J. Zhang, B. Wang, A. Wang, and J. F. Saavedra, Object picture of scalar field perturbation on kerr black hole in scalar-einstein-gauss-bonnet theory, Physical Review D 102
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J. L. Ripley, N. Loutrel, E. Giorgi, and F. Pretorius, Numerical computation of second-order vacuum perturbations of kerr black holes, Physical Review D 103
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A. Zenginoğlu, A null infinity layer for wave scattering, arXiv preprint arXiv:2111.14217 (2021)
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