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Tunnelling Effect and Hawking Radiation from a Vaidya Black Hole

Jun Ren·Jingyi Zhang·Zheng Zhao
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Abstract

In this paper, we extend Parikh' work to the non-stationary black hole. As an example of the non-stationary black hole, we study the tunnelling effect and Hawking radiation from a Vaidya black hole whose Bondi mass is identical to its mass parameter. We view Hawking radiation as a tunnelling process across the event horizon and calculate the tunnelling probability. We find that the result is different from Parikh's work because $\frac{dr_{H}}{dv}$ is the function of Bondi mass m(v).

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Jun Ren, Jingyi Zhang, Zheng Zhao. 2006-06-15. Tunnelling Effect and Hawking Radiation from a Vaidya Black Hole. https://doi.org/10.1088/0256-307x%2F23%2F8%2F016

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