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
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
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.
HUANG Chao-Guang. Spherically Symmetric Static Solution for a Schwarzschild Black Hole with Its Hawking Radiation[J]. 中国物理快报, 2000, 17(5): 329-331.
HUANG Chao-Guang. Spherically Symmetric Static Solution for a Schwarzschild Black Hole with Its Hawking Radiation. Chin. Phys. Lett., 2000, 17(5): 329-331.
2000, Vol. 17 
