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Modulated Natural Inflation

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arxiv 1511.05560 v1 pith:TNIPSUMZ submitted 2015-11-17 hep-th astro-ph.COhep-ph

classification hep-thastro-ph.COhep-ph
keywords inflationalignednaturalpowerstringaxionaxionicby-product
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We discuss some model-independent implications of embedding (aligned) axionic inflation in string theory. As a consequence of string theoretic duality symmetries the pure cosine potentials of natural inflation are replaced by modular functions. This leads to "wiggles" in the inflationary potential that modify the predictions with respect to CMB-observations. In particular, the scalar power spectrum deviates from the standard power law form. As a by-product one can show that trans-Planckian excursions of the aligned effective axion are compatible with the weak gravity conjecture.

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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. Extra-dimensional Origins of Chemical Potentials at the Cosmological Collider

    hep-ph 2026-07 conditional novelty 7.0 of 10

    A rolling 5D gauge-field inflaton acts as an extra-dimensional electric field, creating charged and neutral KK particles far heavier than H and yielding observable oscillatory signatures.

  2. Oscillating scalar fields and the Hubble tension: a resolution with novel signatures

    astro-ph.CO 2019-08 conditional novelty 7.0 of 10

    A subdominant oscillating scalar field with about 10% energy density at redshift 3500 and a potential ∝ φ^{2n} (n≈3) can resolve the Hubble tension, with CMB-S4-detectable polarization signatures and self-resonance for n≈2.

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