Multiscale hydro simulations with Radiative Transfer and (diverse) AGN feedback

Test different physical processes for black hole fuelling and related AGN activity in cosmological, hydrodynamical simulations. Develop and implement new models for mechanical AGN feedback in state-of-the-art, magneto-hydrodynamical simulations inclusive of cosmic rays. Investigate how the radiation emitted by the AGN couples to the interstellar medium by solving the full radiative transfer equation. Follow self-consistently the chemical evolution of the gas phase. Compare predictions from multiscale simulations for the connection between AGN evolution, host galaxy properties and large-scale environment with observations.