The thermodynamic second law in the evaporating black hole space-time
is examined in the context of the two-dimensional dilaton black hole.
The dynamical evolution of entropy is investigated by using the analyt
ical perturbation method and the numerical method. It is shown that th
e thermodynamic second law holds in the vicinity of infalling shell an
d in the region far from the infalling shell in the case of the semi-c
lassical CGHS model. The analysis of general models is also presented
and its implication is discussed.