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
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