  The black hole information paradox is really a combination of two problems:
the causality paradox and the entanglement problem. The causality paradox
arises because in the semiclassical approximation infalling matter gets
causally trapped inside its own horizon; it is therefore unable to send its
information back to infinity if we disallow propagation outside the light cone.
We show how the causality paradox is resolved in the fuzzball paradigm. One
needs to distinguish between two kinds of Rindler spaces: (a) Rindler space
obtained by choosing accelerating coordinates in Minkowski space and (b)
`pseudo-Rindler' space, which describes the region near the surface of a
fuzzball. These two spaces differ in their vacuum fluctuations. While low
energy waves propagate the same way on both spaces, infalling objects with
energies $E\gg T$ suffer an `entropy enhanced tunneling' in the pseudo-Rindler
spacetime (b); this leads to the nucleation of a fuzzball before the infalling
object gets trapped inside a horizon.
