Poster Title:  Supermassive black holes in constrained cosmological hydrodynamic simulations
Poster Abstract: 

We study the early growth of supermassive black holes using constrained realization cosmological simulations. The technical part is twofold: the initial condition generator and the hydrodynamic solver. We use an initial condition generator parallelized in MPI to generate constrained Gaussian realizations to feed in the hydrodynamic solver. The hydrodynamic solver we use for the cosmological simulations is a smooth particle hydrodynamics (SPH) based code also parallelized with MPI. 

Poster ID:  C-4
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