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  Axisymmetric Stability of Kerr Black Holes

Schutz, B. F., & Friedman, J. L. (1974). Axisymmetric Stability of Kerr Black Holes. Physical Review Letters, 32(5), 243-245. doi:10.1103/PhysRevLett.32.243.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-7344-9 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-7347-3
Genre: Journal Article

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60516.pdf (Publisher version), 521KB
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 Creators:
Schutz, Bernard F.1, 2, Author           
Friedman, John L.3, Author
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, ou_24013              
2External Organizations, Yale University, New Haven, Connecticut, ou_persistent22              
3External Organizations, ou_persistent22              

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 Abstract: A variational expression is used to prove that all axisymmetric modes of the Kerr sequence of rotating black holes are stable.

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 Dates: 1974-02-04
 Publication Status: Issued
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 Rev. Type: Peer
 Identifiers: eDoc: 60516
DOI: 10.1103/PhysRevLett.32.243
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Title: Physical Review Letters
Source Genre: Journal
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Pages: - Volume / Issue: 32 (5) Sequence Number: - Start / End Page: 243 - 245 Identifier: ISSN: 1079-7114