QCD Axion Dark Matter with a Small Decay Constant
arXiv:1711.10486 · doi:10.1103/PhysRevLett.120.211602
Abstract
The QCD axion is a good dark matter candidate. The observed dark matter abundance can arise from misalignment or defect mechanisms, which generically require an axion decay constant GeV (or higher). We introduce a new cosmological origin for axion dark matter, parametric resonance from oscillations of the Peccei-Quinn symmetry breaking field, that requires GeV. The axions may be warm enough to give deviations from cold dark matter in Large Scale Structure.
6 pages, 2 figures; v2: discussions and references added
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