Black Hole Radiation inside Apparent Horizon in Quantum Gravity : Astrophysics and Relativity
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概要
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We study black hole radiation inside the apparent horizon in quantum gravity. First we perform a canonical quantization for a spherically symmetric geometry, where one of the spatial coordinates is treated as the time variable, since we would like to consider the interior region of a black hole. Next this rather general formalism is applied for a specific model, where the ingoing Vaidya metric is used as a simple model of an evaporating black hole. Following Tomimatsu's idea, we will analytically solve the Wheeler-DeWitt equation in the vicinity of the apparent horizon and see that the mass-loss rate of a black hole due to thermal radiation is equal to the result obtained by Hawking in his semiclassical treatment. The present formalism may have a wide application in quantum gravity inside the horizon of a black hole to problems such as mass inflation, strong cosmic censorship, etc.
- 理論物理学刊行会の論文
- 1997-02-25
著者
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HOSOYA Akio
Department of Physics, Osaka University
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Hosoya A
Tokyo Inst. Technol. Tokyo Jpn
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Hosoya Akio
Department Of Physics Tokyo Institute Of Technology
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ODA Ichiro
Edogawa University
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Hosoya Akio
Department Of Physics Faculty Of Science Tokyo Institute Of Technology
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ODA Ichiro
Department of Physics, Ochanomizu University
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HOSOYA Akio
Research Institute for Theoretical Physics, Hiroshima University
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HOSOYA Akio
Department of Physics, Osasa University
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