We consider a variant of the brans-world model in which the universe is the
direct product of a Friedmann-Robertson-Walker (FRW) space and a compact h
yperbolic manifold of dimension d greater than or equal to2. Cosmology in t
his space is particularly interesting. The dynamical evolution of the space
-time leads to the injection of a large entropy into the observable (FRW) u
niverse. The exponential dependence of surface area on distance in hyperbol
ic geometry makes this initial entropy very large, even if the CHM has a re
latively small diameter (in fundamental units). The very large statistical
averaging inherent in the collapse of the initial entropy onto the brane ac
ts to smooth out initial inhomogeneities. This smoothing is then sufficient
to account for the current homogeneity of the universe. With only mild fin
e-tuning, the current flatness of the universe can also then be understood.
Finally, recent brane-world approaches to the hierarchy problem can be rea
dily realized within this framework.