A Minimal Sub-Planckian Axion Inflation Model with Large Tensor-to-Scalar Ratio
arXiv:1407.7471 · doi:10.1088/1475-7516/2015/01/018
Abstract
We present a minimal axion inflation model which can generate a large tensor-to-scalar ratio while remaining sub-Planckian. The modulus of a complex scalar field with a potential couples directly to the gauge field of a strongly-coupled sector via a term of the form . This generates a minimum of the potential which is aperiodic in the phase. The resulting inflation model is equivalent to a chaotic inflation model. For the natural case of a leading-order portal-like interaction , the model is equivalent to a chaotic inflation model and predicts a tensor-to-scalar ratio and a scalar spectral index . The value of remains sub-Planckian throughout the observable era of inflation, with for when .
arXiv commentOne minor alteration. Version to be published in JCAP
References in corpus (17)
- BICEP2 I: Detection Of B-mode Polarization at Degree Angular Scales
- Planck 2013 results. XXII. Constraints on inflation
- Monodromy in the CMB: Gravity Waves and String Inflation
- Gravity Waves and Linear Inflation from Axion Monodromy
- What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
- Completing Natural Inflation
- N-flation
- Natural Chaotic Inflation in Supergravity
- A Natural Framework for Chaotic Inflation
- An Ignoble Approach to Large Field Inflation
- BICEP2 II: Experiment and Three-Year Data Set
- A review of Axion Inflation in the era of Planck
- Dante's Inferno
- Aligned Natural Inflation: Monodromies of two Axions
- BICEP2 implications for single-field slow-roll inflation revisited
- Discovery of Large Scale Tensor Mode and Chaotic Inflation in Supergravity
- Sub-Planckian Two-Field Inflation Consistent with the Lyth Bound
Cited by in corpus (12)
- Trajectories with suppressed tensor-to-scalar ratio in Aligned Natural Inflation
- Helical Phase Inflation
- Symmetry Breaking Indication for Supergravity Inflation in Light of the Planck 2015
- The two-field regime of natural inflation
- Perspective on completing natural inflation
- Signatures of Planck Corrections in a Spiralling Axion Inflation Model
- Power spectrum oscillations from Planck-suppressed operators in effective field theory motivated monodromy inflation
- Multi-field inflation and the field-space metric
- New- vs. chaotic-inflations
- The Upper Bound on the Tensor-to-Scalar Ratio Consistent with Quantum Gravity
- Flavored axion-monodromy inflation
- The (relative) size does not matter in inflation