Six Dimensional Streaming Algorithm for Cluster Finding in N-Body Simulations
Aidan Reilly (1), Nikita Ivkin (2,*), Gerard Lemson (1), Vladimir, Braverman (1), and Alexander Szalay (1) ((1) Johns Hopkins University, (2), Amazon, *This work was done while the author was at Johns Hopkins University)

TL;DR
This paper introduces a six-dimensional streaming algorithm that incorporates velocity information to improve cluster detection in N-body simulations, enabling identification of overlapping halos that positional methods miss.
Contribution
The paper presents a novel six-dimensional streaming algorithm that includes velocity data, enhancing cluster detection accuracy in cosmological N-body simulations.
Findings
Successfully detects overlapping halos in simulations
Outperforms previous positional-only methods
Identifies halos indistinguishable in positional space
Abstract
Cosmological N-body simulations are crucial for understanding how the Universe evolves. Studying large-scale distributions of matter in these simulations and comparing them to observations usually involves detecting dense clusters of particles called "halos,'' which are gravitationally bound and expected to form galaxies. However, traditional cluster finders are computationally expensive and use massive amounts of memory. Recent work by Liu et al (Liu et al. (2015)) showed the connection between cluster detection and memory-efficient streaming algorithms and presented a halo finder based on heavy hitter algorithm. Later, Ivkin et al. (Ivkin et al. (2018)) improved the scalability of suggested streaming halo finder with efficient GPU implementation. Both works map particles' positions onto a discrete grid, and therefore lose the rest of the information, such as their velocities.…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena
