Moving Mirror Model of Hawking Evaporation
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概要
- 論文の詳細を見る
The moving mirror model is designed to extract essential features of the black hole formation and the subsequent Hawking radiation by neglecting complication due to a finite curvature. We extend this approach to dynamically treat back reaction against the mirror motion due to the Hawking radiation. It is found that a unique model in two space-time dimensions exists in which the Hawking radiation completely stops and the end point of evaporation contains a disconnected remnant. When viewed from asymptotic observers at one side of the space-time, quantum mechanical correlation is recovered in the end. Although the thermal stage accompanying short range correlation may last for an arbitrarily long period, at a much longer time scale a long tail of non-thermal correlation is clearly detected.
- 理論物理学刊行会の論文
- 1994-05-25
著者
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Yoshimura M
Ritsumeikan Univ. Kusatsu Jpn
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Yoshimura Motohiko
Department Of Physics Tohoku University
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Yoshimura M
Tohoku Univ. Sendai Jpn
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Yoshimura Motohiko
Department Of Physics Okayama University
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YOSHIMURA Motohiki
Department of Physics, Tohoku University
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HOTTA Masahiro
Department of Physics, Tohoku University
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SHINO Masato
Department of Physics, Tohoku University
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Shino Masato
Department Of Physics Tohoku University
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Hotta Masahiro
Department Of Chemistry And Materials Science Tokyo Institute Of Technology
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YOSHIMURA Motohiko
Department of Physics, Tohoku University
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YOSHIMURA Masaki
Department of Physics, Ritsumeikan University
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