  After the gravity induced on the brane in the Randall-Sundrum (RS) infinite
braneworld is briefly reviewed, we discuss the possibility that black holes
evaporate as a result of classical evolution in this model based on the AdS/CFT
correspondence. If this possibility is really the case, the existence of
long-lived solar mass black holes will give the strongest constraint on the
bulk curvature radius. At the same time, we can propose a new method to
simulate the evaporation of a 4D black hole due to the Hawking radiation as a
5D process.
