We examine the cosmology and hierarchy of scales in models with branes imme
rsed in a five-dimensional curved spacetime subject to radion stabilization
. When the radion field is time-independent and the inter-brane spacing is
stabilized, the universe can naturally find itself in the radiation-dominat
ed epoch. This feature is independent of the form of the stabilizing potent
ial. We recover the standard Friedmann equations without assuming a specifi
c form for the bulk energy-momentum tensor. In the models considered, if th
e observable brane has positive tension, a solution to the hierarchy proble
m requires the presence of a negative tension brane somewhere in the bulk.
We find that the string scale can be as low as the electroweak scale. In th
e situation of self-tuning branes where the bulk cosmological constant is s
et to zero, the brane tensions have hierarchical values. In the case of a p
olynomial stabilizing potential no new hierarchy is created. (C) 2000 Publi
shed by Elsevier Science B.V.