Quantum thermal effect of nonstatic charged black hole.

Physics

Scientific paper

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Black Holes: Hawking Radiation

Scientific paper

The difficulty of calculating energy-momentum tensors is avoided by finding directly the solution of the Klein-Gordon and Dirac equations near the horizon. Both the location of the event horizon and the Hawking radiation temperature of a nonstatic charged black hole are shown. The results indicate that the Hawking radiation temperature can be regarded as a compensating effect under the time-scale transformation.

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