About this document
Eddington Limit and Black Hole Growth by cccc36631 is a document available to read on EtoBox.
This document explores how a modified Eddington-limited accretion model, incorporating the Klein-Nishina effect, can explain the rapid growth of supermassive black holes (SMBHs) in the early universe. The authors argue that a geometrically thick, hot quasi-spherical flow allows black holes to grow quickly while still adhering to the Eddington limit, potentially reducing formation time by up to 47%. They propose that a 10 M☉ black hole could evolve into a 10^9 M☉ black hole within 500 million years through a
- Author
- cccc36631
- Language
- EN