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On Hawking Radiation as Tunneling with Back-Reaction

A. J. M. Medved, Elias C. Vagenas

gr-qcarXiv:gr-qc/0504113

Abstract

Recently, Angheben et.al. [hep-th/0503081] have presented a refined method for calculating the (tree-level) black hole temperature by way of the tunneling paradigm. In the current letter, we demonstrate how their formalism can be suitably adapted to accommodate the (higher-order) effects of the gravitational back-reaction.

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