Closed Universes With Black Holes But No Event Horizons As a Solution to   the Black Hole Information Problem
  We show it is possible for the information paradox in black hole evaporation to be resolved classically. Using standard junction conditions, we attach the general closed spherically symmetric dust metric to a spacetime satisfying all standard energy conditions but with a single point future c-boundary. The resulting Omega Point spacetime, which has NO event horizons, nevertheless has black hole type trapped surfaces and hence black holes. But since there are no event horizons, information eventually escapes from the black holes. We show that a scalar quintessence field with an appropriate exponential potential near the final singularity would give rise to an Omega Point final singularity. 
Frank J. Tipler, Jessica Graber, Matthew McGinley, Joshua   Nichols-Barrer, and Christopher Staecker