Hoop Conjecture and Black Holes on a Brane
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概要
- 論文の詳細を見る
The initial data of gravity for a cylindrical matter distribution confined to a brane are studied in the framework of the single-brane Randall-Sundrum scenario. In this scenario, the 5-dimensional nature of gravity appears in the short-range gravitational interaction. We find that a sufficiently thin configuration of matter leads to the formation of a marginal surface, even if the configuration is infinitely long. This implies that the hoop conjecture proposed by Thorne does not hold on the brane: Even if a mass M does not become compacted into a region whose circumference C in every direction satisfies C > 4πGM, black holes with horizons can form in the Randall-Sundrum scenario.
- 理論物理学刊行会の論文
- 2003-03-28
著者
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NAKAO Ken-ichi
Department of Physics, Graduate School of Science, Osaka City University
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Mishima T
Laboratories Of Physics College Of Science And Technology Nihon Universitiy
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Mishima Takashi
Department Of Physics Tokyo Institute Of Technology
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NAKAMURA Kouji
Division of Theoretical Astrophysics, National Astronomical Observatory
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MISHIMA Takashi
Laboratories of Physics, College of Science and Technology, Nihon Universitiy
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Nakao Ken-ichi
Department Of Physics Graduate School Of Science Osaka City University
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Nakao Ken-ichi
Department Of Mathematics And Physics Graduate School Of Science Osaka City University
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Nakamura Kouji
Division Of Theoretical Astrophysics National Astronomical Observatory
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MISHIMA Takashi
Department of Physics, Tokyo Institute of Technology
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