Super-Eddington accretion in protogalactic cores

[2508.21114] Super-Eddington accretion in protogalactic cores Skip to main content We gratefully acknowledge support from the Simons Foundation, member institutions , and all contributors.
Super-Eddington (SE) accretion has emerged as a promising mechanism to solve this issue, yet its impact on early BH evolution in tailored numerical experiments remains largely unexplored.
Our results show that SE accretion naturally leads to BHs that are over-massive relative to their host galaxy stellar content, consistent with JWST observations.
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