Perspective on completing natural inflation
arXiv:1410.1762 · doi:10.3389/fphy.2014.00083
Abstract
We present a perspective on the inflation paths in 2-, 3-,,, N-flation models based on the ultraviolet completion in heterotic string theory, where a number of grand unification scale axions are used. The number of non-Abelian gauge groups for a natural inflation is restricted in string compactification, and we argue that the most plausible completion of natural inflation from a theory perspective is the 2-flation.
5 pages, 1 eps figure
References in corpus (11)
- A Mini-Landscape of Exact MSSM Spectra in Heterotic Orbifolds
- The Heterotic Road to the MSSM with R parity
- Natural inflation with multiple sub-Planckian axions
- Flipped SU(5) from Z_{12-I} orbifold with Wilson line
- Aligned Natural Inflation: Monodromies of two Axions
- Natural Inflation: Consistency with Cosmic Microwave Background Observations of Planck and BICEP2
- From strings to the MSSM
- Helical Phase Inflation
- A Minimal Sub-Planckian Axion Inflation Model with Large Tensor-to-Scalar Ratio
- The inflation point in U(1) hilltop potential assisted by chaoton, BICEP2 data, and trans-Planckian decay constant
- R-symmetric Axion/Natural Inflation in Supergravity via Deformed Moduli Dynamics