The flaw in the firewall argument

A lot of confusion surrounds the issue of black hole complementarity, because the question has been considered without discussing the mechanism which guarantees unitarity. Considering such a mechanism leads to the following: (1) The Hawking quanta with energy E of order the black hole temperature T   carry information, and so only appropriate processes involving E≫TE≫T quanta can have any possible complementary description with an information-free horizon; (2) The stretched horizon describes all possible black hole states with a given mass M  , and it must expand out to a distance sbubblesbubble before it can accept additional infalling bits; (3) The Hawking radiation has a specific low temperature T  , and infalling quanta interact significantly with it only within a distance sαsα of the horizon. One finds sα≪sbubblesα≪sbubble for E≫TE≫T, and this removes the argument against complementarity recently made by Almheiri et al. In particular, the condition E≫TE≫T leads to the notion of ‘fuzzball complementarity’, where the modes around the horizon are indeed correctly entangled in the complementary picture to give the vacuum.