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Are Extremal 2D Black Holes Really Frozen ?

arXiv:hep-th/0012134 · doi:10.1016/S0370-2693(01)00242-8

Abstract

In the standard methodology for evaluating the Hawking radiation emanating from a black hole, the background geometry is fixed. Trying to be more realistic we consider a dynamical geometry for a two-dimensional charged black hole and we evaluate the Hawking radiation as tunneling process. This modification to the geometry gives rise to a nonthermal part in the radiation spectrum. We explore the consequences of this new term for the extremal case.

7 pages, LaTeX, no figures