| Home > Publications database > A New Source for (QCD) Axion Dark Matter Production: Curvature-Induced |
| Preprint | PUBDB-2025-00965 |
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2025
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Please use a persistent id in citations: doi:10.3204/PUBDB-2025-00965
Report No.: DESY-25-033; arXiv:2503.04880
Abstract: We discuss a novel mechanism for generating dark matter from a fast-rolling scalar field, relevant for both inflation and rotating axion models, and apply it specifically to the (QCD) axion. Dark matter comes from scalar field fluctuations generated by the product of the curvature perturbation and the fast-rolling background field. These fluctuations can explain the totality of dark matter in a vast axion parameter space, particularly for the QCD axion, which will be targeted by upcoming experiments. We review the constraints on this mechanism and potential gravitational-wave signatures.
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