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| Preprint | PUBDB-2020-00857 |
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2020
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Please use a persistent id in citations: doi:10.3204/PUBDB-2020-00857
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. Here 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.
Keyword(s): inflaton: field equations ; inflaton: coupling ; black hole: primordial ; power spectrum: scalar ; resonance: enhancement ; gauge field theory ; inflation ; axion ; Chern-Simons term ; back reaction ; nonlinear ; collapse ; velocity
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Conference Presentation
Resonant backreaction in axion inflation
DESY Virtual Theory Forum, DESYHamburg, DESY, Germany, 22 Sep 2020 - 25 Sep 2020
[10.3204/PUBDB-2020-03544]
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Journal Article
Resonant backreaction in axion inflation
DESY Virtual Theory Forum, HamburgHamburg, Germany, 22 Sep 2020 - 25 Sep 2020
Journal of cosmology and astroparticle physics 2009(09), 009 (1-31) (2020) [10.1088/1475-7516/2020/09/009]
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