  In this paper we determine the one loop radiative correction to the higgs
potential due to quantum fluctuations about the background metric of
Randall-Sundrum model. We then examine the effects of the one loop effective
potential on the stability of the classical vacuum paying particular attention
to the tadpole terms which could dominate over the classical potential for
small field configurations. We find that although the one loop potential due to
scale fluctuations could develop a tadpole term in certain regions of the
parameter space, it is positive for either sign of H. The quadratic and quartic
terms in the radiative correction are too small to cause any instability to the
classical vacuum for field configurations that do not violate the limits of
ordinary perturbation theory.
