This is a project which is currently making use of HPC facilities at Newcastle University. It is active.
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Magneto-hydrodynamic simulations of galactic outflows powered by AGN. Simulations feature cosmic ray transport. which will be used to test their impact on outflow dynamics, multi-phase structure and for the production of mock radio images.
The project involves the performance of galaxy evolution simulations with the moving-mesh magneto-hydrodynamic code Arepo (Springel et al. 2010, Pakmor et al. 2016). The code solves for MHD, cosmic ray transport and gravity on an unstructured mesh that advects with the flow.