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Production and backreaction of massive fermions during axion inflation with non-Abelian gauge fields

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abstract

We study the production and backreaction of massive vector-like fermions in the background of a classical SU(2) gauge field during axion-driven inflation. We demonstrate all ultraviolet divergences due to the interactions with the fermions can be absorbed by renormalization of the axion wavefunction and the gauge coupling. The effects of the fermion-axion interaction vanish in the massless limit as required by symmetry. For very massive fermions, contact interactions are induced between the axion, the gauge field and the gravitational field. In this massive limit, we find the usual axion-gauge field interactions are induced, however, in addition we observe the appearance of axion self-interactions, as well as kinetic braiding of the axion with the Einstein tensor. These new axion derivative interactions present intriguing opportunities for model building and phenomenology.

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astro-ph.CO 1

years

2024 1

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CONDITIONAL 1

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Kinetic Gauge Friction in Natural Inflation

astro-ph.CO · 2024-11-29 · conditional · novelty 7.0

Kinetic gauge friction can sustain natural inflation with sub-Planckian f, and a Chern-Simons term stabilizes the perturbations, yielding CMB-compatible spectra.

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  • Kinetic Gauge Friction in Natural Inflation astro-ph.CO · 2024-11-29 · conditional · none · ref 84 · internal anchor

    Kinetic gauge friction can sustain natural inflation with sub-Planckian f, and a Chern-Simons term stabilizes the perturbations, yielding CMB-compatible spectra.