  We apply the recent results in Loop Quantum Cosmology and in the resolution
of Black Hole singularity to the gravitational collapse of a star. We study the
dynamic of the space time in the interior of the Schwarzschild radius. In
particular in our simple model we obtain the evolution of the matter inside the
star and of the gravity outside the region where the matter is present. The
boundary condition identify an unique time inside and outside the region where
the matter is present. We consider a star during the collapse in the particular
case in which inside the collapsing star we take null pressure, homogeneity and
isotropy. The space-time outside the matter is homogeneous and anisotropic. We
show that the space time is singularity free and that we can extend dynamically
the space-time beyond the classical singularity.

General Relativity and Quantum Cosmology