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A Cosmological Mechanism for Stabilizing Moduli

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arxiv hep-th/0001112 v2 pith:Y3OEGCFX submitted 2000-01-19 hep-th astro-phhep-ph

A Cosmological Mechanism for Stabilizing Moduli

classification hep-th astro-phhep-ph
keywords dilatonmechanismmodulifieldspotentialstabilizingcorrectcosmological
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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In this paper, we show how the generic coupling of moduli to the kinetic energy of ordinary matter fields results in a cosmological mechanism that influences the evolution and stability of moduli. As an example, we reconsider the problem of stabilizing the dilaton in a non-perturbative potential induced by gaugino condensates. A well-known difficulty is that the potential is so steep that the dilaton field tends to overrun the correct minimum and to evolve to an observationally unacceptable vacuum. We show that the dilaton coupling to the thermal energy of matter fields produces a natural mechanism for gently relaxing the dilaton field into the correct minimum of the potential without fine-tuning of initial conditions. The same mechanism is potentially relevant for stabilizing other moduli fields.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Curvature-Assisted Dynamical Compactification in a Pre-Inflationary Higher-Dimensional Universe

    hep-th 2026-04 unverdicted novelty 6.0

    Negative curvature sustains tracker-like radion evolution in a 5D open FRW universe, enabling trapping into a compactified vacuum via Casimir and Kaluza-Klein thermal effects before 4D inflation dilutes curvature remnants.

  2. Curvature-Assisted Dynamical Compactification in a Pre-Inflationary Higher-Dimensional Universe

    hep-th 2026-04 unverdicted novelty 4.0

    In a 5D open FRW model, negative curvature sustains tracker-like radion evolution that enables dynamical compactification via Casimir stabilization before 4D inflation dilutes curvature remnants.