Abstract:
If the evaporation of a black hole formed from a pure state is unitary, the entanglement
entropy of the Hawking radiation should follow the Page curve, increasing from zero until near
the halfway point of the evaporation, and then decreasing back to zero. The general argument
for the Page curve is based on the assumption that the quantum state of the black hole plus
radiation during the evaporation process is typical. We show that the Page curve can result
from a simple dynamical input in the evolution of the black hole, based on a recently proposed
signature of quantum chaos, without resorting to typicality. One key feature which leads to
the Page curve is the possibility of dynamical processes where operators which make up the
reduced density operator of a black hole can “jump” outside the black hole, which we refer to as
void formation processes. Such processes are initially exponentially suppressed, but dominate
after a certain time scale, which can be used as a dynamical definition of the Page time. We
conjecture that void formation may provide a microscopic explanation for the recent semi-
classical prescription of including islands in the calculation of the entanglement entropy of the
black hole radiation.