Tunnelling Effect and Hawking Radiation from a Vaidya Black Hole
REN Jun, ZHANG Jing-Yi, ZHAO Zheng
Department of Physics, Beijing Normal University, Beijing 100875
Tunnelling Effect and Hawking Radiation from a Vaidya Black Hole
REN Jun;ZHANG Jing-Yi;ZHAO Zheng
Department of Physics, Beijing Normal University, Beijing 100875
关键词 :
04.70.Dy ,
04.70.-s
Abstract : We extend Parikh’s study to the non-stationary black hole. As an example of the non-stationary black hole, we investigate the tunnelling effect and Hawking radiation from a Vaidya black hole whose Bondi mass is identical to its mass parameter. The Hawking radiation is considered as a tunnelling process across the event horizon and we calculate the tunnelling probability. It is found that the result is different from Parikh’s study because drH /dv is the function of Bondi mass m(v).
Key words :
04.70.Dy
04.70.-s
出版日期: 2006-08-01
:
04.70.Dy
(Quantum aspects of black holes, evaporation, thermodynamics)
04.70.-s
(Physics of black holes)
引用本文:
REN Jun;ZHANG Jing-Yi;ZHAO Zheng. Tunnelling Effect and Hawking Radiation from a Vaidya Black Hole[J]. 中国物理快报, 2006, 23(8): 2019-2022.
REN Jun, ZHANG Jing-Yi, ZHAO Zheng. Tunnelling Effect and Hawking Radiation from a Vaidya Black Hole. Chin. Phys. Lett., 2006, 23(8): 2019-2022.
链接本文:
https://cpl.iphy.ac.cn/CN/
或
https://cpl.iphy.ac.cn/CN/Y2006/V23/I8/2019
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