ELUCID-DESI I: A Parallel MPI Implementation of the Initial Condition Solver for Large-Scale Reconstruction Simulations
Wensheng Hong, Xiaohu Yang, Junde Li, Huiyuan Wang, Zhao Chen, Hong-Ming Zhu, Qingyang Li, Yizhou Gu, Youcai Zhang, Feng Shi, Jiaxin Han, Yu Yu, Zhongxu Zhai

TL;DR
This paper introduces a scalable MPI-parallelized framework for reconstructing cosmic initial conditions, significantly reducing computational costs and enabling large-scale simulations for upcoming cosmological surveys.
Contribution
The authors develop a parallel implementation of the initial condition solver that scales efficiently and includes a novel 'guess' module for rapid high-quality initial density field generation.
Findings
Nearly linear scaling with particles and CPU cores.
Substantial reduction in computational steps and hours for large simulations.
Enabling practical large-volume reconstructions for future surveys.
Abstract
We present a highly scalable, MPI-parallelized framework for reconstructing the initial cosmic density field, designed to meet the computational demands of next-generation cosmological simulations, particularly the upcoming ELUCID-DESI simulation based on DESI BGS data. Building upon the Hamiltonian Monte Carlo approach and the FastPM solver, our code employs domain decomposition to efficiently distribute memory between nodes. Although communication overhead increases the per-step runtime of the MPI version by roughly a factor of eight relative to the shared-memory implementation, our scaling tests-spanning different particle numbers, core counts, and node layouts-show nearly linear scaling with respect to both the number of particles and the number of CPU cores. Furthermore, to significantly reduce computational costs during the initial burn-in phase, we introduce a novel ``guess''…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astrophysics and Star Formation Studies · Cosmology and Gravitation Theories
