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Moduli Stabilization and Inflation Using Wrapped Branes

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arxiv hep-th/0505098 v2 pith:4MUBRO2S submitted 2005-05-11 hep-th astro-phgr-qchep-ph

Moduli Stabilization and Inflation Using Wrapped Branes

classification hep-th astro-phgr-qchep-ph
keywords earlymoduliwrappedbranebranescontextcosmologicaldomain
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We demonstrate that a gas of wrapped branes in the early Universe can help resolve the cosmological Dine-Seiberg/Brustein-Steinhardt overshoot problem in the context of moduli stabilization with steep potentials in string theory. Starting from this mechanism, we propose a cosmological model with a natural setting in the context of an early phase dominated by brane and string gases. The Universe inflates at early times due to the presence of a wrapped two brane (domain wall) gas and all moduli are stabilized. A natural graceful exit from the inflationary regime is achieved. However, the basic model suffers from a generalized domain wall/reheating problem and cannot generate a scale invariant spectrum of fluctuations without additional physics. Several suggestions are presented to address these issues.

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