On the equations governing the gravitational perturbations of the Kerr black hole
- 20 August 1976
- journal article
- Published by The Royal Society in Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences
- Vol. 350 (1661) , 165-174
- https://doi.org/10.1098/rspa.1976.0101
Abstract
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.Keywords
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