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Quantum tunneling and back reaction. (English) Zbl 1282.83025

Summary: We give a correction to the tunneling probability by taking into account the back reaction effect to the metric of the black hole spacetime. We then show how this gives rise to the modifications in the semiclassical black hole entropy and Hawking temperature. Finally, we reproduce the familiar logarithmic correction to the Bekenstein-Hawking area law.

MSC:

83C57 Black holes
81T20 Quantum field theory on curved space or space-time backgrounds
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References:

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