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Instability in axion inflation with strong backreaction from gauge modes

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arxiv 2209.08131 v2 pith:TUUUR2HZ submitted 2022-09-16 astro-ph.CO hep-phhep-th

classification astro-ph.COhep-phhep-th
keywords gaugeinflatonfieldmodesvelocitybackreactioninstabilitystrong
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

We perform an analytical study of the stability of the background solution of the model in which an inflaton, through an axionic coupling to a $U(1)$ gauge field, causes an amplification of the gauge field modes that strongly backreact on its dynamics. To this goal, we study the evolution of the gauge field modes coupled to the inflaton zero mode, treating perturbatively the deviation of the inflaton velocity from its mean-field value. As long as the system is in the strong backreaction regime we find that the inflaton velocity performs oscillations of increasing amplitude about the value it would have in the approximation of constant velocity, confirming an instability that has been observed in numerical studies.

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Cited by 11 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. Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation

    astro-ph.CO 2026-07 conditional novelty 7.0 of 10

    Nonlinear axion-U(1) inflation, simulated on a lattice and fed into N-body simulations, boosts small-scale structure and high-redshift halo counts by up to ~200% relative to standard single-field initial conditions.

  3. Gravitational wave anisotropies from axion inflation

    astro-ph.CO 2025-04 conditional novelty 7.0 of 10

    The sourced gravitational wave background from axion inflation carries energy-density anisotropies up to O(10^{-1}), far larger than the vacuum contribution, due to modulation of sourced tensor modes by CMB-scale curv...

  4. Searching for Inflationary Physics with the CMB Trispectrum: 1. Primordial Theory & Optimal Estimators

    astro-ph.CO 2025-02 conditional novelty 7.0 of 10

    A set of quasi-optimal CMB trispectrum estimators is derived for local, EFT, direction-dependent, spinning-particle, point-source, and lensing templates, enabling first collider searches.

  5. Kinetic Gauge Friction in Natural Inflation

    astro-ph.CO 2024-11 conditional novelty 7.0 of 10

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

  6. 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.

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

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

    Axion inflation with a sufficiently massive vector boson can enter the strong backreaction regime smoothly, avoiding the instability that plagues the massless case.

  8. Axion USR Inflation

    astro-ph.CO 2025-07 conditional novelty 6.0 of 10

    In axion inflation with an intermediate ultra-slow-roll phase, the instability parameter collapses at the start of USR, terminating gauge production and yielding a two-peak power spectrum with P_R ∝ k^m, m>4.

  9. Pure Chromo-Natural Inflation: Signatures of Particle Production from Weak to Strong Backreaction

    astro-ph.CO 2025-04 conditional novelty 6.0 of 10

    Pure chromo-natural inflation unavoidably transitions from weak to strong backreaction, producing a chiral three-peak gravitational wave spectrum and a scalar peak that can form primordial black holes.

  10. 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.

  11. CMB constraints on $U(1)$ axion warm inflation

    astro-ph.CO 2025-07 conditional novelty 4.0 of 10

    Axion-driven warm inflation with U(1) gauge fields is constrained with CMB data and remains viable for sub-Planckian decay constants, but requires large Chern-Simons couplings.

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