Shift Symmetry and Inflation in Supergravity
Philippe Brax, Jerome Martin

TL;DR
This paper explores supergravity inflation models with shift symmetry, demonstrating how mild symmetry breaking can alleviate the eta-problem and produce phenomenologically viable inflationary trajectories.
Contribution
It introduces a novel combination of shift symmetry, moduli stabilization, and symmetry breaking superpotentials to construct inflation models with curved trajectories in supergravity.
Findings
Shift symmetry creates a flat inflaton direction.
Mild symmetry breaking lifts the flatness, alleviating the eta-problem.
Models exhibit curved inflationary trajectories similar to mutated hybrid inflation.
Abstract
We consider models of inflation in supergravity with a shift symmetry. We focus on models with one moduli and one inflaton field. The presence of this symmetry guarantees the existence of a flat direction for the inflaton field. Mildly breaking the shift symmetry using a superpotential which depends not only on the moduli but also on the inflaton field allows one to lift the inflaton flat direction. Along the inflaton direction, the eta-problem is alleviated. Combining the KKLT mechanism for moduli stabilization and a shift symmetry breaking superpotential of the chaotic inflation type, we find models reminiscent of ``mutated hybrid inflation'' where the inflationary trajectory is curved in the moduli--inflaton plane. We analyze the phenomenology of these models and stress their differences with both chaotic and hybrid inflation.
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