The main objective of this report is to
examine {\em if} and {\em how}
the inclusion of supersymmetry
in a quantum cosmological scenario
may add to our
understanding of structure formation in the very early universe.
In this report we
advance the current
repertoire of quantum cosmological models to
incorporate inhomogenous field modes
in a supersymmetric manner. In particular, we introduce
perturbations about a
supersymmetric FRW model.
A quantum state of our model
has properties typical of the
{\em no-boundary} (Hartle--Hawking) proposal. This solution
may then lead to a scale--free spectrum of density perturbations.