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Perturbatively including inhomogeneities in axion inflation

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arxiv 2310.09186 v2 pith:NBCHU2MM submitted 2023-10-13 astro-ph.CO hep-ph

classification astro-ph.COhep-ph
keywords axionfieldregimeinhomogeneitiesgaugeinflationperturbativeabelian
verification ladder T0 review T1 audit T2 compute T3 formal
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Axion inflation, i.e. an axion-like inflaton coupled to an Abelian gauge field through a Chern-Simons interaction, comes with a rich and testable phenomenology. This is particularly true in the strong backreaction regime, where the gauge field production heavily impacts the axion dynamics. Lattice simulations have recently demonstrated the importance of accounting for inhomogeneities of the axion field in this regime. We propose a perturbative scheme to account for these inhomogeneities while maintaining high computational efficiency. Our goal is to accurately capture deviations from the homogeneous axion field approximation within the perturbative regime as well as self-consistently determine the onset of the non-perturbative regime.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Axion Inflation: Perturbative control in the strong backreaction regime

    astro-ph.CO 2026-08 conditional novelty 7.0 of 10

    Axion inflation with strong gauge-field backreaction is generically non-perturbative for ξ ≳ 2.5, yet a newly found steady 'mild backreaction' phase at large β can stay perturbatively controlled.

  2. High-frequency gravitational waves from axion inflation in the weak-backreaction regime

    hep-ph 2026-07 conditional novelty 6.0 of 10

    Even in the weak-backreaction regime, axion inflation produces high-frequency primordial gravitational waves many orders of magnitude above the vacuum spectrum, peaking around MHz–GHz.

  3. Comparative study of the strong backreaction regime in axion inflation: the effect of the potential

    astro-ph.CO 2025-05 conditional novelty 5.0 of 10

    In lattice simulations of axion inflation, the strong-backreaction stage that lengthens inflation occurs for all seven tested potentials, but its duration varies strongly with the potential.

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