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Some Properties of Multi-Component Axion Dark Matter (2510.22569v1)

Published 26 Oct 2025 in hep-ph and astro-ph.CO

Abstract: We introduce a mechanism for multi-component dark matter (DM) that originates from axion mixing. In this context, multi-component DM implies that the cold DM is composed of the QCD axion and many ultra-light axion-like particles (ALPs). This framework can be realized in the type IIB string axiverse with hierarchical axion masses and decay constants. Our investigation reveals that in the light QCD axion scenario, the energy density of the lightest ALP often dominates after mixing, invalidating the canonical light axion scenario. On the other hand, in the heavy QCD axion scenario, both the QCD axion and non-lightest ALPs may dominate, depending on the ALP decay constants. Under certain conditions, the canonical heavy axion scenario remains valid. Finally, we briefly discuss a theoretical framework featuring $\sim\mathcal{O}(100)$ axions, with hierarchical axion masses and decay constants.

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