HACC: Simulating Sky Surveys on State-of-the-Art Supercomputing Architectures
Salman Habib, Adrian Pope, Hal Finkel, Nicholas Frontiere, Katrin, Heitmann, David Daniel, Patricia Fasel, Vitali Morozov, George Zagaris, Tom, Peterka, Venkatram Vishwanath, Zarija Lukic, Saba Sehrish, and Wei-keng Liao

TL;DR
HACC is a versatile, high-performance cosmology simulation code capable of running large-scale universe models efficiently on diverse supercomputing architectures, aiding in understanding dark matter, dark energy, and primordial perturbations.
Contribution
This paper introduces HACC, a new scalable N-body simulation framework optimized for various supercomputers, enabling unprecedented large-scale cosmological simulations.
Findings
Successfully simulated over 3.6 trillion particles.
Demonstrated high efficiency across multiple supercomputing architectures.
Achieved accurate modeling of large-scale cosmic structures.
Abstract
Current and future surveys of large-scale cosmic structure are associated with a massive and complex datastream to study, characterize, and ultimately understand the physics behind the two major components of the 'Dark Universe', dark energy and dark matter. In addition, the surveys also probe primordial perturbations and carry out fundamental measurements, such as determining the sum of neutrino masses. Large-scale simulations of structure formation in the Universe play a critical role in the interpretation of the data and extraction of the physics of interest. Just as survey instruments continue to grow in size and complexity, so do the supercomputers that enable these simulations. Here we report on HACC (Hardware/Hybrid Accelerated Cosmology Code), a recently developed and evolving cosmology N-body code framework, designed to run efficiently on diverse computing architectures and to…
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