  We apply techniques recently introduced in quantum cosmology to the
Schwarzschild metric inside the horizon and near the black hole singularity at
r = 0. In particular, we use the quantization introduced by Husain and Winkler,
which is suggested by Loop Quantum Gravity and is based on an alternative to
the Schrodinger representation introduced by Halvorson. Using this quantization
procedure, we show that the black hole singularity disappears and spacetime can
be dynamically extended beyond the classical singularity.
