Generalizing Kerr-Schild to non-null vectors yields finite curvature expansions, with Ricci-flatness requiring the deformation vector to be irrotational.
On relativistic wave equations for particles of arbitrary spin in an electromagnetic field
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Superradiant clouds around Kerr black holes amplify stochastic gravitational-wave backgrounds via stimulated emission, with rate depending on boson mass and potentially enhancing signals by orders of magnitude.
citing papers explorer
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Generalized Kerr-Schild gauge
Generalizing Kerr-Schild to non-null vectors yields finite curvature expansions, with Ricci-flatness requiring the deformation vector to be irrotational.
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Stimulated Emission from Boson Clouds
Superradiant clouds around Kerr black holes amplify stochastic gravitational-wave backgrounds via stimulated emission, with rate depending on boson mass and potentially enhancing signals by orders of magnitude.