Perturbations of Kerr-de Sitter Black Holes and Heun's Equations : Astrophysics and Relativity
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概要
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It is well known that the perturbation equations of massless fields for the Kerr-de Sitter geometry can be written in the form of separable equations. The equations have five definite singularities, so it has been thought that their analysis would be difficult. we show that these equations can be transformed into Heun's equations, for which we are able to use a known technique to analyze solutions. we reproduce known results for the Kerr geometry and de Sitter geometry in the confluent limits of Heun's functions. Our analysis can be extended to Kerr-Newman-de Sitter geometry for massless fields with spin 0 and 1/2.
- 理論物理学刊行会の論文
- 1998-09-25
著者
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鈴木 久男
北大理
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Takasugi E
Osaka Univ.
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TAKASUGI Eiichi
Department of Physics, Osaka University
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UMETSU Hiroshi
Department of Physics, Osaka University
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Umetsu Hiroshi
Department Of Physics Graduate School Of Science Tohoku University
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Takasugi Eiichi
Department Of Physics Graduate School Of Science Osaka University
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TAKASUGI Eiichi
Department of Physics, Osaka University:Department of Physics, Hokkaido University
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TAKASUGI Eiichi
Institute of Physics, College of General Education, Osaka University
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SUZUKI Hisao
Institute of Physics, College of General Education Osaka University
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Suzuki Hisao
Departmennt of Materials Science, Shizuoka University, 3-5-1 Johoku, Hamamatsu 432-8561, Japan
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Umetsu Hiroshi
Department of Physics,Osaka University
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