摘要
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.
作者
HUANG Chao-Guang
黄超光(Institute of High Energy Physics,Chinese Ac&demy of Sciences,Beijing 100039;Institute of Theoretical Physics,Chinese Academy of Sciences,Beijing 100080)
基金
Supported in part by the National Natural Science Foundation of China under Grant No.19675046
the Climbing up Program of Department of Science and Technology of China.