  We present a new cosmological model derived from Loop Quantum Gravity. The
formulation is based on a projection of the kinematical Hilbert space of the
full theory down to a subspace representing the proper arena for an
inhomogeneous Bianchi I model. This procedure gives a direct link between the
full theory and its cosmological sector. The emerging quantum cosmological
model represents a simplified arena on which the complete canonical
quantization program can be tested. The achievements of this analysis could
also shed light on Loop Quantum Cosmology and its relation with the full
theory.
