Gravitational Radiation from a Naked Singularity : Odd-Parity Perturbation : Astrophysics and Relativity

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概要

• 論文の詳細を見る

• It has been suggested that a naked singularity is a good candidate for a strong gravitational wave burster. A naked singularity occurs in the generic collapse of an inhomogeneous dust ball. We study the odd-parity mode of gravitational waves from a naked singularity of the Lemaitre-Tolman-Bondi spacetime. The wave equation for gravitational waves is solved by numerical integration using the single null coordinate. It is found that the naked singularity is not a strong source of the odd-parity gravitational radiation, although the metric perturbation grows in the central region. Therefore, the Cauchy horizon in this spacetime should be marginally stable with respect to odd-parity perturbations.

• 理論物理学刊行会の論文
• 1999-06-25

著者

• NAKAO Ken-ichi

  Department of Physics, Graduate School of Science, Osaka City University

• Harada Tomohiro

  Department of Cardiovascular Medicine, University of Tokyo

• Harada Tomohiro

  Department Of Cardiovascular Medicine Graduate School Of Medicine University Of Tokyo

• 原田 融

  Sapporo Gakuin Univ. Ebetsu Jpn

• Harada T

  Department Of Physics Waseda University

• Nakano K

  Department Of Physics Osaka City University

• IGUCHI Hideo

  Department of Physics, Tokyo Institute of Technology

• Nakao Ken-ichi

  Department Of Mathematics And Physics Graduate School Of Science Osaka City University

• 原田 融

  札幌学院大

• Igughi Hideo

  Department Of Physics Tokyo Institute Of Technology

• Harada Tomohiro

  Department Of Applied Analysis And Complex Dynamical Systems Graduate School Of Informatics Kyoto Un

• IGUCHI Hideo

  Department of Physics, Kyoto University

• HARADA Toru

  Department of Social Information, Sapporo Gakuin University:Institute of Socio-Information and Communication Studies (ISICS) University of Tokyo

• NAKANO Katsuya

  Department of Computational Science, Faculty of Science, Kanazawa University

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