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Enhanced Early Galaxy Formation in JWST from Axion Dark Matter?

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arxiv 2307.10302 v2 pith:4EZ34YJP submitted 2023-07-18 hep-ph astro-ph.COastro-ph.HEhep-th

classification hep-phastro-ph.COastro-ph.HEhep-th
keywords formationaxiondarkearlyenhancedexistinggalaxyjwst
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abstract

We demonstrate that enhanced early galaxy formation can generically arise in axion-like particle (ALP) dark matter (DM) models with a delayed onset of axion field oscillation. In these models, the formation of localized massive objects enhances structure formation, potentially addressing the excess recently observed by the James Webb Space Telescope (JWST), while remaining consistent with existing constraints. We identify viable parameter space with the ALP mass in the range of $10^{-22}~{\rm eV}<m_a<10^{-19}~\rm eV$. In addition, we show that the ALP parameter regions of interest can lead to intriguing complementary signatures in the small-scale structure of DM halos and existing experimental searches for ALPs.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Early Galaxies from Rare Inflationary Processes and JWST Observations

    astro-ph.CO 2025-02 conditional novelty 6.0 of 10

    Rare Poisson processes during inflation can seed dense regions that collapse into massive galaxies at redshifts where standard cosmology predicts almost none, and JWST could detect them.

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