  We present a new effective description of macroscopic Kruskal black holes
that incorporates corrections due to quantum geometry effects of loop quantum
gravity. It encompasses both the `interior' region that contains classical
singularities and the `exterior' asymptotic region. Singularities are naturally
resolved by the quantum geometry effects of loop quantum gravity, and the
resulting quantum extension of the full Kruskal space-time is free of all the
known limitations of previous investigations [1-11] of the Schwarzschild
interior. We compare and contrast our results with these investigations and
also with the expectations based on the AdS/CFT duality [12].
