On the equations governing the gravitational perturbations of the Kerr black hole

Astronomy and Astrophysics – Astronomy

Scientific paper

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Black Holes (Astronomy), Gravitational Effects, Perturbation Theory, Transformations (Mathematics), Wave Equations, Field Theory (Physics), Metric Space, Potential Theory

Scientific paper

Teukolsky's radial equation governing the general, non-axisymmetric,
gravitational perturbations of the Kerr black hole is reduced to the
form of a one-dimensional wave equation by making use of the
transformation which enables the treatment of the non-axisymmetric modes
in exactly the same way as the axisymmetric modes.

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