We have applied GAMER to several cutting-edge astrophysical simulations. For example, the left figure shows a merging galaxy clusters with a spatial resolution almost an order of magnitude higher than the previous work. This will allow astrophysicists, for the first time, to resolve the turbulence cascade in the intracluster medium on scales comparable to Chandra observations. The right figure shows an isolated disk galaxy simulation aiming for producing a dynamically evolving interstellar medium, undergoing repeated cycles of collapse, star formation, feedback, rarefaction, and re-collapse which have not been fully resolved previously in a global galactic scale simulation.
Project Members: Hsi-Yu Schive, Matthew Turk, Nathan Goldbaum
Collaborators: John ZuHone (Harvard-Smithsonian Center for Astrophysics)
Publications:
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