Abstract

It is well known that large Hubble-induced supergravity corrections to the inflaton field can ruin the flatness of the potential, thus creating a tension between slow-roll inflation and supergravity. In this paper we show that it is possible to obtain a {\it cosmologically flat} direction, embedded within the minimal supersymmetric standard model, despite very large super-Hubble corrections. As an illustration, we show that a flat direction which is lifted by an n=6n=6 operator matches the current cosmic microwave background data for a wide range of the Hubble parameter, 105GeV≲Hinf≲108.510^{5} {\rm GeV}\lesssim H_{inf}\lesssim 10^{8.5} GeV. Our approach can be applied to any FF-term inflationary model.

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