pith. sign in

arxiv: hep-th/0505098 · v2 · submitted 2005-05-11 · ✦ hep-th · astro-ph· gr-qc· hep-ph

Moduli Stabilization and Inflation Using Wrapped Branes

classification ✦ hep-th astro-phgr-qchep-ph
keywords earlymoduliwrappedbranebranescontextcosmologicaldomain
0
0 comments X
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.