  We consider the quantization of the complete extension of the Schwarzschild
space-time using spherically symmetric loop quantum gravity. We find an exact
solution corresponding to the semi-classical theory. The singularity is
eliminated but the space-time still contains a horizon. Although the solution
is known partially numerically and therefore a proper global analysis is not
possible, a global structure akin to a singularity-free Reissner--Nordstr\"om
space-time including a Cauchy horizon is suggested.
