Every year we invite leading experts to share their perspective on the frontiers of computational fluid dynamics and particle-based methods. This year’s keynote lectures reflect both the growing overlap between SPH and mainstream CFD, and the expanding reach of numerical methods more broadly: from the fundamental challenges of multispecies turbulent flow simulations, to the new opportunities opened by exascale computing for SPH in computational astrophysics, to the continued evolution of the δ-SPH scheme family in tackling complex free-surface and multiphase flow problems — the latter presented by this year’s Monaghan Prize recipient.