Post Inflationary Behaviour of String Moduli

TL;DR

This paper investigates the evolution and stabilization mechanisms of string moduli fields after inflation, proposing models that ensure their stabilization at low energies through specific potential features and transition dynamics.

Contribution

It introduces explicit models for moduli stabilization post-inflation, analyzing potential forms and transition mechanisms that improve understanding of moduli dynamics.

Findings

High energy minima stabilization under certain modular weight restrictions

Explicit examples of coinciding minima and smooth transition mechanisms

Reduction of modulus amplitude depends on low energy potential shape

Abstract

We analyze the behaviour of moduli fields in string effective models between the end of inflation and reheating. The effective moduli potential during this era is derived for a class of simple models. We argue that this potential significantly stabilizes the modulus at its high energy minimum, if some restrictions on modular weights are met. Two mechanisms to further stabilize the moduli to their low energy minima are discussed explicitly: coinciding minima at a point of enhanced symmetry, and the smooth transition from high to low energy minimum by an effective mass term C^2 H^2. For both cases we present explicit examples, and C^2 is found to be O(10) at most. In addition, we show that during a smooth transition the reduction of the modulus amplitude strongly depends on the shape of the low energy potential.