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Quenched Hawking Radiation and the Black Hole Pair-Creation Rate by Yi, Piljin is a scholarly article available to read on EtoBox.

What is Quenched Hawking Radiation and the Black Hole Pair-Creation Rate about?

The main topic of this talk is the Hawking effect when the black holes in question are undergoing a uniform acceleration. The semiclassical effect of the acceleration is most striking when the Hawking temperature equals the acceleration temperature. Within the usual late-time approximation, the natural black hole vacuum is then equivalent to the asymptotically empty Minkowskian vacuum, and the accelerated black hole becomes semiclassically stable against the familiar thermal evaporation. An important application of this phenomenon is found in the problem of charged black hole pair-creation.

Author

Yi, Piljin

Published

1995

Language

EN