Hawking effect of the charged evaporating black hole in de Sitter space.

Computer Science

Scientific paper

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Black Holes: De Sitter Universe

Scientific paper

In this article, through discussing the Klein-Gordon equation which is near the horizon, both the location of the event horizon and the Hawking radiation temperature (back-reaction is considered) of the charged evaporating black hole in de Sitter space are shown directly and exactly. Further the authors get the regulation according to which the Hawking radiation temperature can be regarded as a compensate effect under the time-scale transformation.

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