Rotating Black Hole in Extended Chern-Simons Modified Gravity
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概要
- 論文の詳細を見る
We investigate a slowly rotating black hole in four-dimensional extended Chern-Simons modified gravity. We obtain an approximate solution that reduces to the Kerr solution when a coupling constant vanishes. The Chern-Simons correction effectively reduces the frame-dragging effect around a black hole in comparison with that of the Kerr solution.
- 理論物理学刊行会の論文
- 2009-08-25
著者
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Matsuyama Toyoki
Department Of Physics Nara University Of Education
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Tanda Satoshi
Department Of Applied Physics Hokkaido University:center Of Education And Research For Topological S
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Tanda Satoshi
Department Of Applied Physics Hokkaido University
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Matsuyama Toyoki
Department Of Physics Hokkaido University
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KONNO Kohkichi
Department of Applied Physics, Hokkaido University
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Konno Kohkichi
Department Of Applied Physics Hokkaido University:center Of Education And Research For Topological S
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TANDA Satoshi
Department of Applied Physics, Hokkaido University:Center of Education and Research for Topological Science and Technology, Hokkaido University
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Matsuyama Toyoki
Department of Physics, Nara University of Education
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Konno Kohkichi
Department of Applied Physics, Hokkaido University:Center of Education and Research for Topological Science and Technology, Hokkaido University
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