Towards Natural Inflation in String Theory
arXiv:1407.2562 · doi:10.1103/PhysRevD.92.023515
Abstract
We provide type IIB string embeddings of two axion variants of natural inflation. We use a combination of RR 2 form axions as the inflaton field and have its potential generated by non perturbative effects in the superpotential. Besides giving rise to inflation, the models developed take into account the stabilization of the compact space, both in the KKLT and large volume scenario regimes, an essential condition for any semi-realistic model of string inflation.
LaTeX, 1+26 pages, 2 figures; v2: added refs; v3: corrected a LaTeX problem, where v2 refs were compiled with v1 tex file
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- A Flux-Scaling Scenario for High-Scale Moduli Stabilization in String Theory
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- Axion Monodromy and the Weak Gravity Conjecture
- Planckian Axions in String Theory
- What is the Magnetic Weak Gravity Conjecture for Axions?
- Draining the Swampland
- D-brane Potentials in the Warped Resolved Conifold and Natural Inflation
- Sub-Planckian Two-Field Inflation Consistent with the Lyth Bound
- Systematics of type IIB moduli stabilisation with odd axions
- Observable Chiral Gravitational Waves from Inflation in String Theory
- Early Dark Energy in Type IIB String Theory
- Multifield Dynamics in Higgs-otic Inflation
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- On chromonatural inflation in string theory
- Dimensional oxidation and modular completion of non-geometric type IIB action
- Hypercharge Axion and the Diphoton GeV Resonance
- A no-go theorem for monodromy inflation
- Generalized Clockwork Theory
- Issues in Complex Structure Moduli Inflation
- Magnon Inflation: Slow Roll with Steep Potentials
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- Perspective on completing natural inflation
- N-flation in Supergravity
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- Lensing dispersion of SNIa and small scales of the primordial power spectrum
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- Supersymmetric Inflation from the Fifth Dimension
- Enhancement of the Axion Decay Constant in Inflation and the Weak Gravity Conjecture