Collision of Time-Like Shells in Spherically Symmetric Spacetime : Astrophysics and Relativity
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概要
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The spacetime representing a collision of two time-like shells is studied. This spacetime is constructed by 'cutting and pasting' four distinct Reissner-Nordstrom-de Sitter spacetimes. The junction condition is uniquely determined under the condition that the two colliding shells are transparent. In the limit of the collision of two neutral null shells, the junction condition reduces to the Dray-'t Hooft-Redmount (DTR) relation. The collision near the horizon is also investigated, and it is shown that phenomena like mass inflation do not occur unless one of the colliding shells is escaping from the horizon.
- 理論物理学刊行会の論文
- 1999-05-25
著者
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NAKAO Ken-ichi
Department of Physics, Graduate School of Science, Osaka City University
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IDA Daisuke
Department of Physics, Gakushuin University
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Nakao Ken-ichi
Department Of Mathematics And Physics Graduate School Of Science Osaka City University
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Ida Daisuke
Department Of Physics Gakushuin University
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NAKAO Kenichi
Yukawa Institute for Theoretical Physics, Kyoto University
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IDA Daisuke
Department of Physics, Tokyo Institute, of Technology
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IDA Daisuke
Department of Physics, Kyoto University
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