Conference Presentation PUBDB-2020-03544

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Resonant backreaction in axion inflation

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2020

DESY Virtual Theory Forum, DESYHamburg, DESY, Germany, 22 Sep 2020 - 25 Sep 20202020-09-222020-09-25 [10.3204/PUBDB-2020-03544]  GO

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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. 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.


Note: LaTeX, 1+28 pages, 10 figures

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 2020-09-23, last modified 2021-11-29


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