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Hawking Radiation from a Non-static Black Hole |
ZHAO Zheng;DAI Xianxin |
Department of Physics, Beijing Normal University, Beijing 100875 |
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Cite this article: |
ZHAO Zheng, DAI Xianxin 1991 Chin. Phys. Lett. 8 548-550 |
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Abstract A method exactly determining an event horizon and its temperature in a non-static space-time is proposed. Using the generalized Tortoise coordinate, we give exact location of event horizon and exact Hawking temperature for a general spherically symmetric evaporating black hole.
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Keywords:
97.60.Lf
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Published: 01 October 1991
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Abstract
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