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Stability in Axion Inflation with Strong Backreaction from a Massive Vector Boson

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arxiv 2607.22893 v1 pith:32A5K3YQ submitted 2026-07-24 astro-ph.CO hep-phhep-th

classification astro-ph.COhep-phhep-th
keywords fieldgaugeinflationmassiveaxionbackreactionregimestrong
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abstract

We study a modification of the model of axion inflation coupled to a $U(1)$ gauge field where the vector field is massive. In the conventional scenario with a massless gauge field, the onset of the regime where the gauge field strongly backreacts on the inflaton displays an instability whose nonlinear evolution and endpoint remain poorly understood. We argue that, if the gauge field is massive enough, the transition to the strong backreaction regime instead occurs smoothly, avoiding this instability. This observation suggests that axion inflation with massive gauge fields admits a controllable strong backreaction regime, so that a phenomenologically viable realization of inflation might be possible in this class of models.

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Cited by 2 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. Axion Inflation with a Massive Abelian Gauge Field

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    A massive Abelian gauge field axially coupled to the inflaton yields tachyonic production only for |ξ|>m/H, with sourced CMB curvature power suppressed as ~1/m̄²–1/m̄³ at fixed backreaction, allowing strong friction f...

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