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Potential reconstruction from general power spectrum in single-field inflation

Published 29 Sep 2021 in astro-ph.CO, gr-qc, and hep-ph | (2109.14241v2)

Abstract: We suggest a new method to reconstruct, within canonical single-field inflation, the inflaton potential directly from the primordial power spectrum which may deviate significantly from near scale-invariance. Our approach relies on a more generalized slow-roll approximation than the standard one, and can probe the properties of the inflaton potential reliably. We give a few examples for reconstructing potential and discuss the validity of our method.

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