A Unified Dark-matter-driven Relativistic Bondi Route to Black Hole Growth from Stellar to Supermassive Scales
Observations of luminous quasars at z ≳ 7 reveal supermassive black holes (SMBHs) with inferred masses M _BH ∼ 10 ^9 M _⊙ formed within the first ∼700 Myr of cosmic history. Standard growth channels—Eddington-limited gas accretion and hierarchical mergers—face severe timescale restrictions. We con...
Tallennettuna:
| Päätekijät: | , |
|---|---|
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
IOP Publishing
2026-01-01
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| Sarja: | The Astrophysical Journal Letters |
| Aiheet: | |
| Linkit: | https://doi.org/10.3847/2041-8213/ae5954 |
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