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A real-time, WebGPU-accelerated simulation of the Large-Scale Structure of the Universe. Visualize the evolution of cosmic filaments and voids from z=10 to the present day, powered by 2LPT and quasi-N-body dynamics directly in your browser.
Algorithm for Void Identification in Cosmology is a comprehensive and significant update to a previous void finder published by Ricciardelli et al. (2013). Density and velocity divergence are used to define unstructured voids, which are formed by combining a set of cubes.
Systematic comparison of galaxies in cosmic voids versus dense "walls" using DESI DR1 data to investigate environmental quenching mechanisms in galaxy evolution.