  We consider a broad class of inflationary models of two unconstrained chiral
superfields, the stabilizer $S$ and the inflaton $\Phi$, which can describe
inflationary models with nearly arbitrary potentials. These models include, in
particular, the recently introduced theories of cosmological attractors, which
provide an excellent fit to the latest Planck data. We show that by adding to
the superpotential of the fields $S$ and $\Phi$ a small term depending on a
nilpotent chiral superfield $P$ one can break SUSY and introduce a small
cosmological constant without affecting main predictions of the original
inflationary scenario.
