Super-Eddington accretion in protogalactic cores

The presence of massive black holes (BHs) exceeding 109 M⊙ already at redshift z > 6 challenges standard models of BH growth. 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 largel...

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Autors principals:	Zana Tommaso, Capelo Pedro R., Boresta Mairo, Schneider Raffaella, Lupi Alessandro, Trinca Alessandro, Mayer Lucio, Valiante Rosa, Graziani Luca
Format:	Artigo
Idioma:	Inglês
Publicat:	EDP Sciences 2026-04-01
Col·lecció:	Astronomy & Astrophysics
Matèries:	accretion accretion disks black hole physics methods: numerical galaxies: high-redshift quasars: supermassive black holes
Accés en línia:	https://www.aanda.org/articles/aa/full_html/2026/04/aa57006-25/aa57006-25.html
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