This research paper introduces RAMSES-yOMP, a modified version of the RAMSES astrophysical hydrodynamic simulation code designed for enhanced parallel efficiency. The key innovation lies in incorporating OpenMP (OMP) directives alongside the existing Message Passing Interface (MPI) parallelization, creating a hybrid approach that leverages both shared and distributed memory models.
The study aims to address the computational and memory limitations of RAMSES, particularly when handling large-scale simulations on multi-core systems. The authors seek to improve parallel scalability and optimize resource utilization for enhanced performance.
The researchers implemented OMP directives in time-intensive subroutines, employing static scheduling for grid-based operations and dynamic scheduling for particle-based tasks. They replaced the original Conjugate Gradient (CG) solver with a preconditioned pipelined Conjugate Gradient (PPCG) solver for improved efficiency in gravitational potential calculations. Additionally, they refined the load balancing scheme by adjusting the cost function to better reflect the computational load associated with particles.
Benchmark simulations demonstrated that RAMSES-yOMP, with 16 OMP threads, achieved a two-fold speedup compared to the original RAMSES code. This improvement was attributed to better load balancing, reduced overhead in domain decomposition, and the enhanced Poisson equation solver. Moreover, the hybrid parallelization scheme led to significant reductions in memory usage (up to 77%) and disk space utilization (up to 30%).
The study concludes that hybrid parallelization using OMP and MPI significantly enhances the performance of RAMSES, enabling larger and higher-resolution simulations. The reduced memory footprint allows for efficient resource utilization, making the code suitable for systems with limited RAM capacity.
RAMSES-yOMP offers a valuable tool for astrophysical research, enabling more efficient and detailed simulations of complex phenomena. The improved performance and resource utilization contribute to advancing our understanding of astrophysical processes.
While demonstrating significant improvements, the authors acknowledge potential bottlenecks in particle-based subroutines that require further optimization. Future research could explore alternative parallelization strategies for these specific tasks to further enhance the code's performance.
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