Moduli Stabilization and Inflation Using Wrapped Branes
arXiv:hep-th/0505098 · doi:10.1103/PhysRevD.72.026002
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.
7 pages, 5 figures, REVTeX; References added, note added
References in corpus (25)
- Big Bang Nucleosynthesis (in "The Review of Particle Properties" 2004)
- de Sitter Vacua in String Theory
- Racetrack Inflation
- Challenges for Superstring Cosmology
- Brane Gases in the Early Universe
- Cosmology With Negative Potentials
- Moduli Stabilization with the String Higgs Effect
- Stabilization of Extra Dimensions at Tree Level
- Natural Quintessence and Large Extra Dimensions
- Loitering Phase in Brane Gas Cosmology
- Stabilizing the Dilaton in Superstring Cosmology
- On T-Duality in Brane Gas Cosmology
- Cosmological String Gas on Orbifolds
- Brane Gases on K3 and Calabi-Yau Manifolds
- Inflation and Brane Gases
- Cosmological stabilization of moduli with steep potentials
- Late-time dynamics of brane gas cosmology
- Dilaton Stabilization in Brane Gas Cosmology
- Volume Stabilization and Acceleration in Brane Gas Cosmology
- Stabilization of Embedded Defects by Plasma Effects
- D-brane Gases and Stabilization of Extra Dimensions in Dilaton Gravity
- Coupled Inflation and Brane Gases
- Stabilization of the Electroweak Z String in the Early Universe
- Accelerating universes driven by bulk particles
- Moduli Evolution in Heterotic Scenarios
Cited by in corpus (33)
- String Gas Cosmology
- String Gas Cosmology and Structure Formation
- Volume Modulus Inflation and the Gravitino Mass Problem
- Holes in the walls: primordial black holes as a solution to the cosmological domain wall problem
- More on the Spectrum of Perturbations in String Gas Cosmology
- Moduli Stabilization in String Gas Cosmology
- Moduli Stabilization in Brane Gas Cosmology with Superpotentials
- Stabilizing moduli with thermal matter and nonperturbative effects
- Dark energy and decompactification in string gas cosmology
- Challenges for String Gas Cosmology
- Acceleration of the Universe via f(R) Gravities and The Stability of Extra Dimensions
- Pre-Inflationary Spacetime in String Cosmology
- Cyclic Inflation
- Conceptual Problems of Inflationary Cosmology and a New Approach to Cosmological Structure Formation
- Moduli evolution in the presence of flux compactifications
- Moduli Stabilization in String Gas Compactification
- Stabilization of Compactification Volume In a Noncommutative Mini-Super-Phase-Space
- Supersymmetry Breaking and Dilaton Stabilization in String Gas Cosmology
- The Most Probable Size of the Universe
- S-duality in String Gas Cosmology
- Target space duality and moduli stabilization in String Gas Cosmology
- Early universe in view of a modified theory of gravity
- Lovelock inflation and the number of large dimensions
- Moduli fixing and T-duality in Type II brane gas models
- Stabilization of the Extra Dimensions in Brane Gas Cosmology with Bulk Flux
- The Relic Problem of String Gas Cosmology
- T and S dualities and The cosmological evolution of the dilaton and the scale factors
- Colliding Branes and Formation of Spacetime Singularities
- Radion effective potential in brane gas cosmology
- String Gas Baryogenesis
- Wrapped brane gas as a candidate for Dark Matter
- Extra Dimensions, Dilaton and Dark Energy
- Looking Beyond Inflationary Cosmology