NON-GAUSSIAN ISOCURVATURE PERTURBATIONS FROM INFLATION

We present a class of very simple inflationary models of two scalar fi elds which leads to non-Gaussian isothermal perturbations with a ''blu e'' spectrum, n>1. One of the models is inspired by supersymmetric the ories where light scalar fields naturally acquire masses similar to H during inflation. Another model presumes that one of the fields has a nonminimal interaction with gravity xi R sigma(2). By a slight modific ation of parameters of these models one can obtain either Gaussian iso thermal perturbations, or non-Gaussian adiabatic perturbations with n> 1.