Fuzzy dark matter simulations

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Authors: Hsi-Yu Schive
Cited by: 4
References: 170

Abstract

Abstract Fuzzy dark matter (FDM), composed of ultralight bosons, exhibits intricate wave phenomena on galactic scales. Compared to cold dark matter, FDM simulations are significantly more computationally demanding due to the need to resolve the de Broglie wavelength and its rapid oscillations. In this review, we first outline the governing equations and distinctive features of FDM. We then present a range of numerical algorithms for both wave- and fluid-based simulations, discuss their respective advantages and limitations, and highlight representative test problems. To facilitate code comparison, we also provide publicly available initial condition files for both isolated-halo and cosmological simulations.

Fields of Study & Subjects

Dark Matter and Cosmic Phenomena Computational Physics and Python Applications Cosmology and Gravitation Theories

Publication details

Journal / source
Living Reviews in Computational Astrophysics
Publisher
Springer Science and Business Media LLC
Volume
12
Issue
1
Publication date
2 April 2026
Language
EN