  We study the conditions of restoring supersymmetry (SUSY) after inflation in
the supergravity-based cosmological models with a single chiral superfield and
a quartic stabilization term in the K\"ahler potential. Some new, explicit, and
viable inflationary models satisfying those conditions are found. The
inflaton's scalar superpartner is dynamically stabilized during and after
inflation. We also demonstrate a possibility of having small and adjustable
SUSY breaking with a tiny cosmological constant.
