Gravitational Radiation from a Naked Singularity. II : Even -Parity Perturbation
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概要
- 論文の詳細を見る
A naked singularity occurs in the generic collapse of an inhomogeneous dust ball. We study the even-parity mode of gravitational waves from a naked singularity of the Lemaitre-Tolman-Bondi spacetime. The wave equations for gravitational waves are solved by numerical integration using the single null coordinate. The result implies that the metric perturbation grows when it approaches the Cauchy horizon and diverges there, although the naked singularity is not a strong source of even-parity gravitational radiation. Therefore, the Cauchy horizon in this spacetime should be unstable with respect to linear even-parity perturbations.
- 理論物理学刊行会の論文
- 2000-01-25
著者
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NAKAO Ken-ichi
Department of Physics, Graduate School of Science, Osaka City University
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Harada Tomohiro
Department of Cardiovascular Medicine, University of Tokyo
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Harada Tomohiro
Department Of Cardiovascular Medicine Graduate School Of Medicine University Of Tokyo
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原田 融
Sapporo Gakuin Univ. Ebetsu Jpn
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Harada T
Department Of Physics Waseda University
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Nakano K
Department Of Physics Osaka City University
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IGUCHI Hideo
Department of Physics, Tokyo Institute of Technology
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Nakao Ken-ichi
Department Of Mathematics And Physics Graduate School Of Science Osaka City University
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原田 融
札幌学院大
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Igughi Hideo
Department Of Physics Tokyo Institute Of Technology
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Harada Tomohiro
Department Of Applied Analysis And Complex Dynamical Systems Graduate School Of Informatics Kyoto Un
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IGUCHI Hideo
Department of Physics, Kyoto University
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HARADA Toru
Department of Social Information, Sapporo Gakuin University:Institute of Socio-Information and Communication Studies (ISICS) University of Tokyo
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