ar X iv : h ep - t h / 99 02 18 9 v 2 3 0 M ar 1 99 9 DIAS - STP - 99 - 02 THE DEFORMED TWO - DIMENSIONAL BLACK HOLE
نویسنده
چکیده
A deformation of the wave equation on a two-dimensional black hole is considered as a toy-model for possible gravitational or stringy nonlocal effects. The deformed wave-equation allows for an initial-value problem despite being nonlocal. The singularity present in the classical geometry is resolved by the deformation, so that propagation of a wave-packet can be continued through the classically singular region, ultimately reaching another asymptotically " flat " region.
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