  We propose a general scenario for moduli stabilization where low-energy
supersymmetry can be accommodated with a high scale of inflation. The key
ingredient is that the stabilization of the modulus field during and after
inflation is not associated with a single, common scale, but relies on two
different mechanisms. We illustrate this general scenario in a simple example,
where during inflation the modulus is stabilized with a large mass by a Kahler
potential coupling to the field which provides the inflationary vacuum energy
via its F-term. After inflation, the modulus is stabilized, for instance, by a
KKLT superpotential.
