English

A Minimal Sub-Planckian Axion Inflation Model with Large Tensor-to-Scalar Ratio

High Energy Physics - Phenomenology 2015-06-22 v3 Cosmology and Nongalactic Astrophysics High Energy Physics - Theory

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 Φ\Phi with a λΦ4\lambda |\Phi|^4 potential couples directly to the gauge field of a strongly-coupled sector via a term of the form (Φ/MPl)mFF~(|\Phi|/M_{Pl})^{m} F \tilde{F}. This generates a minimum of the potential which is aperiodic in the phase. The resulting inflation model is equivalent to a ϕ4/(m+1)\phi^{4/(m+1)} chaotic inflation model. For the natural case of a leading-order portal-like interaction ΦΦFF~\Phi^{\dagger}\Phi F \tilde{F}, the model is equivalent to a ϕ4/3\phi^{4/3} chaotic inflation model and predicts a tensor-to-scalar ratio r=16/3N=0.097r = 16/3N = 0.097 and a scalar spectral index ns=15/3N=0.970n_{s} = 1-5/3N = 0.970. The value of Φ|\Phi| remains sub-Planckian throughout the observable era of inflation, with Φ0.01MPl|\Phi| \lesssim 0.01 M_{Pl} for N60N \lesssim 60 when λ1\lambda \sim 1.

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