Intermediate Scale Theory Use Cases

Description of two examples of intermediate scale numerical simulations of very different astrophysical problems. The first problem addresses the evolution of globular clusters, where the dynamical and stellar evolution is followed for every star in the cluster. The second problem describes the evolution of extragalactic jets, both energetic FRII MHD jets and less energetic FRI MHD jets in clusters of galaxies that form buoyant bubbles in the intracluster medium.