  We investigate a particle physics model for cosmic inflation based on the
following assumptions: (i) there are at least two complex scalar fields; (ii)
the scalar potential is bounded from below and remains perturbative up to the
Planck scale; (iii) we assume slow-roll inflation with maximally correlated
adiabatic and entropy fluctuations 50--60 e-folds before the end of inflation.
The energy scale of the inflation is set automatically by the model. Assuming
also at least one massive right handed neutrino, we explore the allowed
parameter space of the scalar potential as a function of the Yukawa coupling of
this neutrino.
