Chandrasekhar, S. ; Detweiler, S. (1976) On the equations governing the gravitational perturbations of the Kerr black hole Proceedings of the Royal Society of London. Series A, Mathematical and Physical Sciences, 350 (1661). pp. 165-174. ISSN 0080-4630
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Official URL: http://www.jstor.org/pss/79047
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.
Item Type: | Article |
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Source: | Copyright of this article belongs to The Royal Society. |
ID Code: | 70834 |
Deposited On: | 22 Nov 2011 04:42 |
Last Modified: | 22 Nov 2011 04:42 |
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