  We extend the ideas introduced in the previous work to a more general
space-time. In particular we consider the Kantowski-Sachs space time with space
section with topology $R \times S^2$. In this way we want to study a general
space time that we think to be the space time inside the horizon of a black
hole. In this case the phase space is four dimensional and we simply apply the
quantization procedure suggested by Loop Quantum Gravity and based on an
alternative to the Schroedinger representation introduced by H. Halvorson.
Through this quantization procedure we show that the inverse of the volume
density and the Schwarzschild curvature invariant are upper bounded and so the
space time is singularity free. Also in this case we can extend dynamically the
space time beyond the classical singularity.
