  Black Holes are unique objects which allow for meaningful theoretical studies
of strong gravity and even quantum gravity effects. An infalling and a distant
observer would have very different views on the structure of the world.
However, a careful analysis has shown that it entails no genuine contradictions
for physics, and the paradigm of observer complementarity has been coined.
Recently this picture was put into doubt. In particular, it was argued that in
old Black Holes a firewall must form in order to protect the basic principles
of quantum mechanics. This AMPS paradox has already been discussed in a vast
number of papers with different attitudes and conclusions. Here we want to
argue that a possible source of confusion is neglection of quantum gravity
effects. Contrary to widespread perception, it does not necessarily mean that
effective field theory is inapplicable in rather smooth neighbourhoods of large
Black Hole horizons. The real offender might be an attempt to consistently use
it over the huge distances from the near-horizon zone of old Black Holes to the
early radiation. We give simple estimates to support this viewpoint and show
how the Page time and (somewhat more speculative) scrambling time do appear.
