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Scalar, vector and tensor perturbations on the Kerr spacetime are governed by equations that can be solved by separation of variables, but the same is not true in generic stationary and axisymmetric geometries.
1901
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F. D. Ryan, “Gravitational waves from the inspiral of a compact object into a massive, axisymmetric body with arbitrary multipole moments,”
1995
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Fintan D. Ryan, “Accuracy of estimating the multipole moments of a massive body from the gravitational waves of a binary inspiral,”
1997
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2001
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2003
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