  We argue certain nonviolent local quantum field theory (LQFT) modification
considered at the global horizon ($r=2M$) of a static spherically-symmetric
black hole can lead to adiabatic leakage of quantum information in the form of
Hawking particles. The source of the modification is (i) smooth at $r=2M$ and
(ii) rapidly vanishing at $r\gg2M$. Furthermore, we restore the unitary
evolution by introducing extra quanta which departs slightly from the generic
Hawking emission without changing the experience of an infalling observer (no
drama). Also, we suggest that a possible interpretation of the
Bekenstein-Hawking bound as entanglement entropy may yield a nonsingular
dynamical horizon behavior described by black hole thermodynamics. Hence by
treating gravity as a field theory, and considering its coupling to the matter
fields in the Minkowski vacuum, we derive the conjectured fluctuations of the
background geometry of a black hole.
