Hawking Effect of Vaidya Black Hole in Higher DimensionalSpace-Time
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Abstract
Making use of the generalized tortoise transformation, the radial part of the Klein-Gordon equation can be reduced to the standard wave equation around the event horizon in the higher dimensional Vaidya space-time. Both the location of event horizon and the radiation temperature of black hole are shown automatically.
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Cite this article:
LI Zhongheng, ZHAO Zheng. Hawking Effect of Vaidya Black Hole in Higher DimensionalSpace-Time[J]. Chin. Phys. Lett., 1994, 11(1): 8-11.
LI Zhongheng, ZHAO Zheng. Hawking Effect of Vaidya Black Hole in Higher DimensionalSpace-Time[J]. Chin. Phys. Lett., 1994, 11(1): 8-11.
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LI Zhongheng, ZHAO Zheng. Hawking Effect of Vaidya Black Hole in Higher DimensionalSpace-Time[J]. Chin. Phys. Lett., 1994, 11(1): 8-11.
LI Zhongheng, ZHAO Zheng. Hawking Effect of Vaidya Black Hole in Higher DimensionalSpace-Time[J]. Chin. Phys. Lett., 1994, 11(1): 8-11.
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