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| Conference Presentation | PUBDB-2020-03544 |
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2020
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Please use a persistent id in citations: doi:10.3204/PUBDB-2020-03544
Report No.: DESY-20-017; arXiv:2002.02952
Abstract: Axion inflation entails a coupling of the inflaton field to gauge fields through the Chern-Simons term. This results in a strong gauge field production during inflation, which backreacts on the inflaton equation of motion. We show that this strongly non-linear system generically experiences a resonant enhancement of the gauge field production, resulting in oscillatory features in the inflaton velocity as well as in the gauge field spectrum. The gauge fields source a strongly enhanced scalar power spectrum at small scales, exceeding previous estimates. For appropriate parameter choices, the collapse of these over-dense regions can lead to a large population of (light) primordial black holes with remarkable phenomenological consequences.
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Resonant backreaction in axion inflation
[10.3204/PUBDB-2020-00857]
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