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Charged Particle Tunnels from the Slowly Varying Reissner--Nordstrom Black Hole |
YANG Shu-Zheng;CHEN De-You |
Institute of Theoretical Physics, China West Normal University, Nanchong 637002 |
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Cite this article: |
YANG Shu-Zheng, CHEN De-You 2007 Chin. Phys. Lett. 24 1479-1481 |
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Abstract Extending Parikh and Wilczek's work to the non-stationary black hole, we discuss the Hawking radiation of the slowly varying Reissner--Nordstrom black hole by considering the unfixed background spacetime and the self-gravitation interaction. The result shows that the tunnelling rate is related to both the variation of Bekenstein--Hawking entropy and the radiation spectrum deviating from the purely thermal one. This is in agreement with Parikh and Wilczek's result. Then a new method to study Hawking radiation of the non-stationary black holes is presented.
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Keywords:
04.70.-s
97.60.Lf
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Received: 14 November 2006
Published: 17 May 2007
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