  We use a new approach to the UV behavior of quantum general relativity,
together with some recent results from the phenomenological asymptotic safety
analysis of the theory, to discuss the final state of the Hawking radiation for
an originally very massive black hole solution of Einstein's theory. We find
that, after the black hole evaporates to the Planck mass size, its horizon is
obviated by quantum loop effects, rendering the entire mass of the originally
massive black hole accessible to our universe.
