The inefficiency of star formation in massive elliptical galaxies is widely believed to be
caused by the interactions of an active galactic nucleus (AGN) with the surrounding gas …

We study the population of supermassive black holes (SMBHs) and their effects on massive
central galaxies in the IllustrisTNG cosmological hydrodynamical simulations of galaxy …

We present a novel implementation of supermassive black hole (SMBH) formation,
dynamics and accretion in the massively parallel tree+ SPH code, ChaNGa. This approach …

We investigate black hole–host galaxy scaling relations in cosmological simulations with a
self-consistent black hole growth and feedback model. Our sub-grid accretion model …

We present Phantom, a fast, parallel, modular, and low-memory smoothed particle
hydrodynamics and magnetohydrodynamics code developed over the last decade for …

We employ hydrodynamical simulations using the moving-mesh code arepo to investigate
the role of energy and momentum input from active galactic nuclei (AGN) in driving large …

By using a set of different star formation rate (SFR) indicators, including Wide-field Infrared
Survey Explorer (WISE) mid-infrared and H α emission, we study the slope of the main …

In this work, we establish and test methods for implementing dynamical friction (DF) for
massive black hole pairs that form in large volume cosmological hydrodynamical …

We introduce a sub-grid force correction term to better model the dynamical friction
experienced by a supermassive black hole (SMBH) as it orbits within its host galaxy. This …

We investigate how the way galaxies acquire their gas across cosmic time in cosmological
hydrodynamic simulations is modified by a comprehensive physical model for baryonic …