Axion kinetic misalignment and parametric resonance from inflation

Raymond T. Co, Lawrence J. Hall, Keisuke Harigaya, Keith A. Olive, Sarunas Verner

Research output: Contribution to journalArticlepeer-review

2 Scopus citations

Abstract

Axion cold dark matter from standard misalignment typically requires a decay constant fa 1011 GeV . Kinetic misalignment and parametric resonance easily allow lower values of fa when the radial Peccei-Quinn (PQ) symmetry breaking field takes large initial values. Here, we consider the effects of inflation on kinetic misalignment and parametric resonance. We assume that the initial PQ field value is determined by quantum fluctuations, and is set by the Hubble parameter during inflation, HI, and the PQ field mass. PQ field oscillations begin before or after the completion of reheating after inflation at a temperature TR. We determine the range of fa and the inflationary parameters (HI, TR) consistent with axion dark matter for a quartic potential for the PQ field. We find that 108 GeV < fa < 1011 GeV can consistently produce axion dark matter. A significant portion of the allowed parameter space predicts rare kaon decays, KL → (π0 + missing energy), and/or suppression of structure formation on small scales.

Original languageEnglish (US)
Article number036
JournalJournal of Cosmology and Astroparticle Physics
Volume2020
Issue number8
DOIs
StatePublished - Aug 2020

Bibliographical note

Publisher Copyright:
© 2020 IOP Publishing Ltd and Sissa Medialab.

Keywords

  • Axions
  • Dark matter theory
  • Particle physics-cosmology connection
  • Physics of the early universe

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