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- W2896651906 abstract "Axions as dark matter is an increasingly important subject in astrophysics and cosmology. Experimental and observational searches are mounting across the mass spectrum of axion-like particles, many of which require detailed knowledge of axion structure over a wide range of scales. Current understanding of axion structures is far from complete, however, due largely to controversy in modeling the candidate's highly-degenerate state. The series Axion Structure Formation seeks to develop a consistent model of QCD axion dark matter dynamics that follows their highly-degenerate nature to the present using novel modeling techniques and sophisticated simulations. This inaugural paper presents the problem of describing many non-relativistic axions with minimal degrees of freedom and constructs a theory of axion infall for the limit of complete condensation. The derived model is shown to contain axion-specific dynamics not unlike the exchange-correlation influences experienced by identical fermions. Perturbative calculations are performed to explore the potential for imprints in early universe structures." @default.
- W2896651906 created "2018-10-26" @default.
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- W2896651906 date "2019-03-02" @default.
- W2896651906 modified "2023-10-11" @default.
- W2896651906 title "Axion structure formation – I: the co-motion picture" @default.
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- W2896651906 doi "https://doi.org/10.1093/mnras/stz488" @default.
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