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Non-Gaussianity from Axion-Gauge Fields Interactions during Inflation

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arxiv 1806.05474 v2 pith:KCDOZPZP submitted 2018-06-14 astro-ph.CO gr-qchep-phhep-th

Emanuela Dimastrogiovanni , Matteo Fasiello , Robert J. Hardwick , Hooshyar Assadullahi , Kazuya Koyama , David Wands This is my paper
classification astro-ph.COgr-qchep-phhep-th
keywords fieldsgaugeinflationalreadyamplitudeaxionaxion-gaugechiral
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We study the scalar-tensor-tensor non-Gaussian signal in an inflationary model comprising also an axion coupled with SU(2) gauge fields. In this set-up, metric fluctuations are sourced by the gauge fields already at the linear level providing an enhanced chiral gravitational waves spectrum. The same mechanism is at work in generating an amplitude for the three-point function that is parametrically larger than in standard single-field inflation.

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  1. 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.

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