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QCD Axion Dark Matter with a Small Decay Constant (1711.10486v2)

Published 28 Nov 2017 in hep-ph and astro-ph.CO

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 $f_a \sim \mathcal{O}(10{11})$ 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 $f_a \sim (108 -10{11})$ GeV. The axions may be warm enough to give deviations from cold dark matter in Large Scale Structure.

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