A Minimal Sub-Planckian Axion Inflation Model with Large Tensor-to-Scalar Ratio
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 .
Keywords
Cite
@article{arxiv.1407.7471,
title = {A Minimal Sub-Planckian Axion Inflation Model with Large Tensor-to-Scalar Ratio},
author = {John McDonald},
journal= {arXiv preprint arXiv:1407.7471},
year = {2015}
}
Comments
One minor alteration. Version to be published in JCAP