Abstract
We numerically analyze the evolution of a two-dimensional dilatonic black hole, within the Callan-Giddings-Harvey-Strominger model. We focus our attention on the finite-mass corrections to the universal evaporation rate which applies at the large-mass limit. Our numerical results confirm a previous theoretical prediction for the first-order ($\ensuremath{\propto}1/M$) correction. In addition, our results strongly suggest that the next-order ($\ensuremath{\propto}1/{M}^{2}$) term vanishes and provide a rough estimate for the third-order term.
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