We present significant evidence in favour of the holographic conjecture that
``4D black holes localized on the brane found by solving the classical bulk
equations in AdS5 are quantum corrected black holes and not classical
ones''. The crucial test is the calculation of the quantum correction to the
Newtonian potential based on a numerical computation of in
Schwarzschild spacetime for matter fields in the zero temperature Boulware
vacuum state. For the case of the conformally invariant scalar field the
leading order term is found to be $M/45\pi r^3$. This result is equivalent to
the result which was previously obtained in the weak-field approximation using
Feynman diagrams and which has been shown to be equivalent, via the AdS/CFT
duality, to the analogous calculation in Randall-Sundrum braneworlds. This
asymptotic behavior was not captured in the analytical approximations for
proposed in the literature. The 4D backreaction equations are then
used to make a prediction about the existence and the possible spacetime
structure of macroscopic static braneworld black holes.Comment: 4 pages, 2 figure