Abstract
The nature of outflows from Supermassive Black Holes (SMBHs) and their impact on the host galaxies are an unresolved question in Black Hole (BH) physics. In order to shed light upon this issue, this project aims at investigating in a self-consistent way the winds produced by SMBHs fed at low and high mass accretion rates. We will use the tools of global, multidimensional MHD simulations o…