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Geometrical Destabilisation of Ultra-Light Axions in String Inflation

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arxiv 1903.01497 v1 pith:UGTR5U2P submitted 2019-03-04 hep-th astro-ph.CO

Geometrical Destabilisation of Ultra-Light Axions in String Inflation

classification hep-th astro-ph.CO
keywords inflationanalysisaxionsdestabilisationevolutionfibregeometricalisocurvature
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We perform a detailed analytical and numerical analysis of the multi-field evolution of Fibre Inflation and show that, regardless of the microscopic realisation of the model, the mass-squared of one of the two ultra-light axions becomes always negative during inflation. This implies that the corresponding isocurvature perturbations experience a potential geometrical destabilisation which seems to bring the system away from the perturbative regime. Therefore we conclude that a full understanding of the inflationary evolution of Fibre Inflation can be achieved only via a non-perturbative analysis where the backreaction of tachyonic isocurvature perturbations is properly taken into account.

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Cited by 3 Pith papers

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

  1. Chiral global embedding of Fibre Inflation with $\overline{\rm D3}$ uplift

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  2. Spectator Axions in String Inflation and Primordial Black Holes

    hep-th 2026-07 conditional novelty 6.0

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  3. Ultra slow-turn inflation

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    In slow-roll multi-field inflation, stability should be read from the total entropy perturbation, which decays in 'ultra slow-turn' models even when the isocurvature effective mass-squared is negative.