Journal Article PUBDB-2020-03826

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Resonant backreaction in axion inflation

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2020
IOP London

DESY Virtual Theory Forum, HamburgHamburg, Germany, 22 Sep 2020 - 25 Sep 20202020-09-222020-09-25 Journal of cosmology and astroparticle physics 2009(09), 009 (1-31) () [10.1088/1475-7516/2020/09/009]
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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 fholes 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 ; gravitation: collapse ; numerical calculations ; cosmological model

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Note: LaTeX, 2+32 pages, 11 figures; appendix C added, version accepted by JCAP

Contributing Institute(s):
  1. Theorie-Gruppe (T)
Research Program(s):
  1. 611 - Fundamental Particles and Forces (POF3-611) (POF3-611)
  2. STRINGFLATION - Inflation in String Theory - Connecting Quantum Gravity with Observations (647995) (647995)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2020
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Resonant backreaction in axion inflation
[10.3204/PUBDB-2020-00857]  GO OpenAccess  Download fulltext Files  Download fulltextFulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS


 Record created 2020-10-14, last modified 2025-07-16