📝 SummarXiv

Abstract

We present a novel, GPU-optimized algorithm for particle-mesh interactions in grid-based hydrodynamics simulations, designed for massively parallel architectures. This approach overcomes the inefficiency of particle neighbour searches or sorts across multiple GPU nodes by using a new ``particle-mesh-particle'' interaction scheme, which extends the particle-mesh method for self-gravity. The algorithm proceeds in two main stages: first, quantities exchanged between particles and the mesh -- such as mass, energy, and momentum added by stellar feedback or removed by accretion onto a sink -- are deposited into a buffer mesh equipped with ghost zones, where multiple contributions per cell are accumulated using atomic additions and then communicated across distributed memory ranks. In the second stage, the buffer states are applied to real mesh states, incorporating cell-wise limiters to enforce physical constraints such as positive density. We implement this scheme in the GPU-native radiation-magnetohydrodynamics code QUOKKA, demonstrating its application to both supernova feedback and sink particle accretion. We demonstrate that the former scheme converges in the terminal radial momentum from multiple supernovae across varying spatial resolutions, while for the latter simulations of accretion in several configurations show excellent agreement with analytic solutions. This scheme enables efficient, scalable particle-mesh coupling for GPU-optimized simulations.