eSSENCE@LU 11:4 - Galaxy formation in the exascale era

As part of our project, we aim to port key multi-scale physical models to DYABLO. The transition to DYABLO presents significant advantages, particularly in terms of potential performance improvements and enhanced support for GPU acceleration. These enhancements are critical for managing the increasing complexity and scale of astrophysical simulations, allowing us to leverage the full power of modern computational resources. Ultimately, we are setting the stage for a groundbreaking achievement: the first-ever simulation of a Milky Way-like galaxy from the Big Bang to the present, with individual stars resolved - a leap far beyond the current limit of grouping stars by tens of thousands.