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Gravitational-wave equation in effective one-body background for spinless binary
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We construct the gravitational-wave equation in the background of the effective one-body system for the spinless binary, which is in general available with the spherically symmetric background as well. The gauge conditions are given in terms of the metric perturbation.
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Teukolsky-like equations with various spins in a deformed Kerr spacetime
On a Kerr spacetime with an arbitrary radial deformation L(r), all massless spin fields satisfy one unified Teukolsky-like master equation that separates into a standard angular part and a deformed radial part.
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