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We discuss how under certain conditions the black hole information puzzle andthe (related) arguments that firewalls are a typical feature of black holes canbreak down. We first review the arguments of AMPS favoring firewalls, focusingon entanglements in a simple toy model for a black hole and the Hawkingradiation. By introducing a large and inaccessible system entangled with theblack hole (representing perhaps a de Sitter stretched horizon or inaccessiblepart of a landscape) we show complementarity can be restored and firewalls canbe avoided throughout the black hole's evolution. Under these conditions blackholes do not have an "information problem". We point out flaws in some of ourearlier arguments that such entanglement might be generically present in somecosmological scenarios, and call out certain ways our picture may still berealized.

No Firewalls or Information Problem for Black Holes Entangled with Large Systems