Outputs (4)

The Three Hundred Project: the evolution of galaxy cluster density profiles (2018)
Journal Article

Recent numerical studies of the dark matter density profiles of massive galaxy clusters (Mhalo > 1015 M) show that their median radial mass density profile remains unchanged up to z > 1, displaying a highly self-similar evolution. We verify this by u... Read More about The Three Hundred Project: the evolution of galaxy cluster density profiles.

The Three Hundred Project: a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications (2018)
Journal Article

We introduce the The Three Hundred project, an endeavour to model 324 large galaxy clusters with full-physics hydrodynamical re-simulations. Here we present the dataset and study the differences to observations for fundamental galaxy cluster properti... Read More about The Three Hundred Project: a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications.

Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models (2018)
Journal Article

We present a comparison of the observed evolving galaxy stellar mass functions with the predictions of eight semi-analytic models and one halo occupation distribution model. While most models are able to fit the data at low redshift, some of them str... Read More about Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models.

An SPH multi-fluid model based on quasi-buoyancy for interface stabilization up to high density ratios and realistic wave speed ratios (2018)
Journal Article

We introduce a Smoothed Particle Hydrodynamics (SPH) concept for the stabilization of the interface between two fluids. It is demonstrated that the change in the pressure gradient across the interface leads to a force imbalance. This force imbalance... Read More about An SPH multi-fluid model based on quasi-buoyancy for interface stabilization up to high density ratios and realistic wave speed ratios.