Ubiquitous seeding of supermassive black holes by direct collapse
We study for the first time the environment of massive black hole (BH) seeds (˜104-5 M⊙) formed via the direct collapse of pristine gas clouds in massive haloes (≥107 M⊙) at z > 6. Our model is based on the evolution of dark matter haloes within a cosmological N-body simulation, combined with prescriptions for the formation of BH along with both
Agarwal, Bhaskar et al.
Fecha de publicación:
10
2012