Natural inflation with natural number of e-foldings

preprint2020arXivOpen access

Abstract

We examine natural inflation without the use of the standard slow-roll approximation by considering the number of physical e-folds ln⁡(aeHe/aH)\ln (a_eH_e/aH). We show that H~=aH∝cos⁡(Aϕ/2)2/A2sin⁡(Aϕ/2)\tilde{H} = aH \propto \cos(A ϕ/2)^{2/A^2} \sin(A ϕ/2) produces a natural inflationary scenario. This model may be solved exactly, showing that the slow-roll approximation overestimates the tensor-to-scalar ratio by about 13−19%13-19 \% for ns≈0.96n_s \approx 0.96 and 50−6050-60 ee-folds.

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