The semiclassical Einstein equation in five dimensions with a negative cosm
ological constant and conformally invariant bulk matter Gelds is examined i
n the brane world scenario with S-1/Z(2) compactification. When numbers N-b
,N-f of bosonic and fermionic fields satisfy I<<kappa>(2)l(-3)(N-b-N-f)<32I
, we obtain an exact semiclassical solution which has two static branes wit
h positive tension and for which the warp factor can be arbitrarily large.
Here, <kappa>(2) is the five-dimensional gravitational constant, l is a len
gth scale determined by the negative five-dimensional cosmological constant
, and I is a dimensionless positive constant of order unity. However, in or
der to obtain a large warp factor, fine-tuning of brane tensions is require
d. Hence, in order to solve the hierarchy problem, we need to justify the f
ine-tuning by another new mechanism.