A possible quick growth mechanism for supermassive black holes
An article published in “The Astrophysical Journal” reports a study on a possible quick growth mechanism of supermassive black holes that could explain their presence when the universe was very young. Ph.D. student at SISSA (International School of Advanced Studies) Lumen Boco and his supervisor Andrea Lapi created a new model based on a process already considered important called dynamical friction in the gaseous medium applying it to multiple mergers.
