The DOI matches its Crossref record; 15 of the 15 references it cites were found in a registry or an index.
An analytic representation for the quasi-normal modes of Kerr black holes
Abstract
The gravitational quasi-normal frequencies of both stationary and rotating black holes are calculated by constructing exact eigensolutions to the radiative boundary-value problem of Chandrasekhar and Detweiler. The method is that employed by Jaffé in his determination of the electronic spectra of the hydrogen molecule ion in 1934, and analytic representations of the quasi-normal mode wavefunctions are presented here for the first time. Numerical solution of Jaffé’s characteristic equation indicates that for each l-pole there is an infinite number of damped Schwarzschild quasi-normal modes. The real parts of the corresponding frequencies are bounded, but the imaginary parts are not. Figures are presented that illustrate the trajectories the five least-damped of these frequencies trace in the complex frequency plane as the angular momentum of the black hole increases from zero to near the Kerr limit of maximum angular momentum per unit mass, a = M, where there is a coalescence of the more highly damped frequencies to the purely real value of the critical frequency for superradiant scattering.
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Citations
Cites
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The quasi-normal modes of the Schwarzschild black hole
Chandrasekhar, S., & Detweiler, S. (1975) · Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences · doi:10.1098/rspa.1975.0112 · Cited by 717
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New approach to the quasinormal modes of a black hole
Ferrari, V., & Mashhoon, B. (1984) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.30.295 · Cited by 585
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Cited by
Quasinormal modes of black holes and black branes
Berti, E., Cardoso, V., & Starinets, A. O. (2009) · Classical and Quantum Gravity · doi:10.1088/0264-9381/26/16/163001 · Cited by 2,095
Quasinormal modes of black holes: From astrophysics to string theory
Konoplya, R. A., & Zhidenko, A. (2011) · Reviews of Modern Physics · doi:10.1103/revmodphys.83.793 · Cited by 1,532
Bohr's Correspondence Principle and the Area Spectrum of Quantum Black Holes
Hod, S. (1998) · Physical Review Letters · doi:10.1103/physrevlett.81.4293 · Cited by 729
Black-hole bomb and superradiant instabilities
Cardoso, V., Dias, Ó. J. C., Lemos, J. P. S., & Yoshida, S. (2004) · Physical Review D · doi:10.1103/physrevd.70.044039 · Cited by 371
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
Metadata
- Authors
- Leaver, E. W.
- Venue
- Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences
- Publisher
- The Royal Society
- Published
- 1985-12-09
- Volume
- 402
- Issue
- 1823
- Pages
- 285-298
- ISSN
- 0080-4630 (ISSN-L)
- 2053-9169
- OpenAlex
- W1968369949
- Cited by
- 1,308
- References
- 15
- FWCI
- 2.96
- Type
- journal article
- Language
- en
- Open access
- closed
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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