
TL;DR
This paper investigates how thermal effects in early universe string cosmology can stabilize moduli fields, avoiding the cosmological moduli problem by dynamically attracting moduli to local minima at enhanced symmetry points.
Contribution
It demonstrates moduli stabilization via thermal effects in heterotic and type II string models, identifying specific points in moduli space where minima occur, and explores duality relations for stabilization.
Findings
Thermal effects induce effective potentials with local minima at symmetry points.
Moduli acquire decreasing masses, diluting scalar oscillations before nucleosynthesis.
Stabilization occurs at enhanced gauge symmetry or shrinking cycle loci in Calabi-Yau spaces.
Abstract
We study moduli stabilization by thermal effects in the cosmological context. The implementation of finite temperature, which spontaneously breaks supersymmetry, induces an effective potential at one loop level. At the points where extra massless states appear in the string spectrum, the potential develops local minima whose depth depends on the temperature. Moduli attracted to these points acquire dynamical masses which decrease with cosmological evolution. This makes the coherent scalar oscillations dilute before nucleosynthesis, and the cosmological moduli problem is avoided. In particular, we study the effective potential induced by a maximally supersymmetric heterotic string gas for spacetime dimension D>=4, and a gas of type II strings compactified on Calabi-Yau three-folds (D=4). In the former case, the local minima of the potential arise at enhanced gauge symmetry points, which…
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