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Perturbations of a Rotating Black Hole
Abstract
Decoupled, separable equations describing perturbations of a Kerr black hole are derived. These equations can be used to study black-hole processes involving scalar, electromagnetic, neutrino or gravitational fields. A number of astrophysical applications are made: Misner's idea that gravitational synchrotron radiation might explain Weber's observations is shown to be untenable; rotating black holes are shown to be stable against small perturbations; energy amplification by superradiant scattering of waves off a rotating black hole is computed; the spin down (loss of angular momentum) of a rotating black hole caused by a stationary non-axisymmetric perturbation is calculated.
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Cited by
Hidden conformal symmetry of the Kerr black hole
Castro, A., Maloney, A., & Strominger, A. (2010) · Physical Review D · doi:10.1103/physrevd.82.024008 · Cited by 295
Curiel, E. (2017) · Einstein Studies · doi:10.1007/978-1-4939-3210-8_3 · Cited by 226
The spectra of gravitational atoms
Baumann, D., Chia, H. S., Stout, J., & Haar, L. T. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/12/006 · Cited by 194
Hawking radiation from a (4+ n )-dimensional black hole: exact results for the Schwarzschild phase
Harris, C. M., & Kanti, P. (2003) · Journal of High Energy Physics · doi:10.1088/1126-6708/2003/10/014 · Cited by 170
Metadata
- Authors
- Teukolsky, S. A.
- Published
- 1974-01-01
- Volume
- 64
- Pages
- 92-92
- OpenAlex
- W3153824498
- Cited by
- 179
- References
- 0
- FWCI
- 0.39
- Type
- journal article
- Language
- en
- Open access
- closed
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- Teukolsky, S. A. (1974). Perturbations of a Rotating Black Hole. https://doi.org/10.1017/s0074180900071011
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
