Tunnelling Effect and Hawking Radiation from a Vaidya Black Hole

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 $\frac{d{r}_H}{dv}$ is the function of Bondi mass m(v).

References in corpus (5)

• Hawking Radiation as Tunneling
• Self-Interaction Correction to Black Hole Radiance
• Radiation via Tunneling from a de Sitter Cosmological Horizon
• Hawking Radiation from AdS Black Holes
• Energy Conservation and Hawking Radiation

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