Inflation and flat directions in modular invariant superstring effective theories
Mary K. Gaillard (UC Berkeley, LBNL), David H. Lyth (Lancaster),, Hitoshi Murayama (UC Berkeley, LBNL)

TL;DR
This paper explores how inflationary potentials can remain flat in string-derived supergravity models, enabling inflation with stabilized moduli and the dilaton, by generalizing no-scale supergravity concepts.
Contribution
It introduces a realistic string-inspired supergravity framework that preserves flat directions during inflation, facilitating moduli stabilization and dilaton control.
Findings
Flat directions are preserved in the proposed supergravity models.
Inflation can occur with a stabilized dilaton and moduli.
The model supports hybrid inflation driven by a Fayet-Illiopoulos term.
Abstract
The potential during inflation must be very flat in, at least, the direction of the inflaton. In renormalizable global supersymmetry, flat directions are ubiquitous, but they are not preserved in a generic supergravity theory. It is known that at least some of them are preserved in no-scale supergravity, and simple generalizations of it. We here study a more realistic generalization, based on string-derived supergravity, using the linear supermultiplet formalism for the dilaton. We consider a general class of hybrid inflation models, where a Fayet-Illiopoulos term drives some fields to large values. The potential is dominated by the term, but flatness is preserved in some directions. This allows inflation, with the dilaton stabilized in its domain of attraction, and some moduli stabilized at their vacuum values. Another modulus may be the inflaton.
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