A Permutation on Hybrid Natural Inflation
Christopher D. Carone, Joshua Erlich, Marc Sher, Raymundo Ramos

TL;DR
This paper explores a hybrid natural inflation model utilizing the S_3 discrete symmetry, leading to a pseudo-Goldstone inflaton with potential for observable tensor modes, while maintaining sub-Planckian field values.
Contribution
It introduces a novel hybrid natural inflation model based on the S_3 symmetry, detailing how this restricts the potential and couplings, and identifies viable parameters with observable tensor modes.
Findings
The model can produce observable tensor-to-scalar ratios r.
The inflaton potential is constrained by S_3 symmetry, ensuring specific form and couplings.
Viable parameter space exists with sub-Planckian inflaton field values.
Abstract
We analyze a model of hybrid natural inflation based on the smallest non-Abelian discrete group S_3. Leading invariant terms in the scalar potential have an accidental global symmetry that is spontaneously broken, providing a pseudo-Goldstone boson that is identified as the inflaton. The S_3 symmetry restricts both the form of the inflaton potential and the couplings of the inflaton field to the waterfall fields responsible for the end of inflation. We identify viable points in the model parameter space. Although the power in tensor modes is small in most of the parameter space of the model, we identify parameter choices that yield potentially observable values of r without super-Planckian initial values of the inflaton field.
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