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Perturbations of a Rotating Black Hole

Published online by Cambridge University Press:  07 February 2017

Saul A. Teukolsky
Saul A. Teukolsky*
Affiliation:
California Institute of Technology, Pasadena, Calif., U.S.A.

Abstract

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Decoupled, separable wave equations describing neutrino, electromagnetic and gravitational perturbations have been derived (Teukolsky, 1972, 1973). A number of applications have been made (Press and Teukolsky, 1973; Starobinsky and Churilov, 1973).

Type
Part II: Stability and Collapse
Information
Symposium - International Astronomical Union , Volume 64: Gravitational Radiation and Gravitational Collapse , 1974 , pp. 92
Copyright
Copyright © Reidel 1974 

References

Press, W. H. and Teukolsky, S. A.: 1973, Astrophys. J. 185, 649.CrossRefGoogle Scholar
Starobinsky, A. A. and Churilov, S. M.: 1973, Zh. E.T.F. 65, 3.Google Scholar
Teukolsky, S. A.: 1972, Phys. Rev. Letters 29, 1114.CrossRefGoogle Scholar
Teukolsky, S. A.: 1973, Astrophys. J. 185, 635.Google Scholar