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  Black-hole normal modes: A WKB approach. III. The Reissner-Nordström black hole

Schutz, B. F., & Kokkotas, K. D. (1987). Black-hole normal modes: A WKB approach. III. The Reissner-Nordström black hole. Physical Review D, 37(12), 3378-3387. doi:10.1103/PhysRevD.37.3378.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-7363-5 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-7367-E
Genre: Journal Article

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61250.pdf (Any fulltext), 987KB
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 Creators:
Schutz, Bernard F.1, 2, Author              
Kokkotas, Kostas D.3, Author
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, escidoc:24013              
2External Organizations, Department of Applied Mathematics and Astronomy, University College, Cardiff, escidoc:persistent22              
3External Organizations, escidoc:persistent22              

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 Abstract: Complex frequencies of the normal modes of the Reissner-Nordström black hole are computed by two independent methods. The first is a high-order WKB approach devised by Schutz and Will and extended by Iyer and Will for the Schwarzschild case. The second is direct numerical integration using a method developed by Chandrasekhar and Detweiler, thereby extending earlier results of Gunter. The WKB results agree with the numerical ones with an error less than 1% for the lowest-order modes. For somewhat higher orders, the numerical techniques fail but the WKB method continues to give eigenfrequencies that should be reasonably accurate.

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 Dates: 1987-06-15
 Publication Status: Published in print
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 Rev. Method: Peer
 Identifiers: eDoc: 61250
DOI: 10.1103/PhysRevD.37.3378
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Title: Physical Review D
Source Genre: Journal
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Pages: - Volume / Issue: 37 (12) Sequence Number: - Start / End Page: 3378 - 3387 Identifier: ISSN: 1089-4918