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Quantum Thermal Effect of Nonstatic Charged Black Hole
Authors:Zhang Lichun  Wu Yueqin  Zhao Ren
Abstract:The difficulty of calculating energy-momentumtensors is avoided by finding directly the solution ofKlein–Gordon and Dirac equations near the horizon.Both the location of the event horizon and the Hawking radiation temperature of a nonstatic chargedblack hole are shown. The results indicate that theHawking radiation temperature can be regarded as acompensating effect under the timescaletransformation.
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