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

preprint2015arXivOpen access

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 ΦΦ with a λ∣Φ∣4λ|Φ|^4 potential couples directly to the gauge field of a strongly-coupled sector via a term of the form (∣Φ∣/MPl)mFF~(|Φ|/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)ϕ^{4/(m+1)} chaotic inflation model. For the natural case of a leading-order portal-like interaction Φ†ΦFF~Φ^{\dagger}ΦF \tilde{F}, the model is equivalent to a ϕ4/3ϕ^{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=1−5/3N=0.970n_{s} = 1-5/3N = 0.970. The value of ∣Φ∣|Φ| remains sub-Planckian throughout the observable era of inflation, with ∣Φ∣≲0.01MPl|Φ| \lesssim 0.01 M_{Pl} for N≲60N \lesssim 60 when λ∼1λ\sim 1.

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