Original Articles |
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Spherically Symmetric Static Solution for a Schwarzschild Black Hole with Its Hawking Radiation |
HUANG Chao-Guang |
Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100039,
and Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100080
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Cite this article: |
HUANG Chao-Guang 2000 Chin. Phys. Lett. 17 329-331 |
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Abstract A black hole and its Hawking radiation may be in stable thermal equilibrium. In this letter, the static spherically symmetric numerical solution for a Schwarzschild black hole with its Hawking radiation are obtained. In the calculation, the equilibrium system is supposed to consist of a black hole, thermal radiation and a two-dimensional surface layer. The solutions obtained are compared with the York’s back-reaction approach and the Zhao-Liu thermodynamic approach.
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Keywords:
04.70.Dy
97.60.Lf
04.20.Jb
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Published: 01 May 2000
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PACS: |
04.70.Dy
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(Quantum aspects of black holes, evaporation, thermodynamics)
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97.60.Lf
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(Black holes)
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04.20.Jb
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(Exact solutions)
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