Critical Behavior of Black Hole Formation in a Scalar Wave Collapse
スポンサーリンク
概要
- 論文の詳細を見る
We present a self-similar model of spherically symmetric collapse of a massless scalar field with a parameter p. The black hole formation is explicitly shown to occur only in the strong-field implosion of p>1. The field evolution in the critical limit p→1 is compared with numerical results found by Choptuik.
- 理論物理学刊行会の論文
- 1994-06-25
著者
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NAKAMURA Kouji
Department of Astronomical Science, The Graduate University for Advanced Studies
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NAKAMURA Kouji
Division of Theoretical Astrophysics, National Astronomical Observatory
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冨松 彰
名大・理
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TOMIMATSU Akira
Department of Physics, Nagoya University
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冨松 彰
名古屋大 理
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冨松 彰
名古屋大理
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Nakamura K
National Astronomical Observatory Mitaka Jpn
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OSHIRO Yoshimi
Department of Physics, Nagoya University
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Oshiro Yoshimi
Department Of Physics Nagoya University
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Tomimatsu Akira
Department Of Physics Kyoto University Kyoto Research Institute For Fundamental Physics Kyoto Univer
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Nakamura K
Division Of Theoretical Astrophysics National Astronomical Observatory
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Tomimatsu Akira
Research Institute For Technical Physics Hiroshima University
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Tomimatsu Akira
Department Of Physics Kyoto University
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Nakamura Kouji
Department Of Applied Biological Chemistry Faculty Of Agriculture Niigata University
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TOMIMATSU Akira
Department of Physics, University of Nagoya
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TOMIMATSU Akira
Research Institute for Theoretical Physics, Hiroshima University
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TOMIMATSU Akira
Research Institute for Theoretical Physics, Hiroshima Universtiy
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NAKAMURA Ken
Deparment of Physics, Rikkyo University
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