Neural Network Fast-Tracks Galaxy Formation express

Original: "A graph-based Neural Network surrogate model for accelerating semi-analytical model of galaxy formation and evolution"
arXiv:2604.23147 · 2026-04-25 · CC BY 4.0 · 1 min
Artificial intelligence now predicts galaxy properties from the history of dark matter growth.

📄 Showing the "Simple" version — "Popular" is not ready yet. Add it to favorites to help prioritize it.

Studying the birth of galaxies requires simulating billions of years of dark matter growth and star formation — even supercomputers handle this slowly. The solution came from machine learning: a neural network, like a seasoned pastry chef, from the 'recipe' of dark matter mergers instantly evaluates the future galaxy — its mass, brightness, chemical composition. Training on thousands of virtual universes led to an almost perfect match with real calculations.

The model was trained on data from the Uchuu simulation and covers almost the entire history of the cosmos — from the young Universe to the present day.

An unexpected finding: the details of internal processes turned out to be secondary. A galaxy's fate is almost entirely written in its dark matter history. Accuracy reaches 97%, and speed allows testing thousands of expansion of the universe scenarios in hours, bringing us closer to understanding cosmic evolution.

The most distant galaxies formed when the Universe was less than a billion years old. Their fate was sealed only by the mergers of invisible dark matter — visible stars simply followed this script.

Like Asimov's 'psychohistory,' the neural network predicts the fate of galaxies through mathematical patterns — only here, it's dark matter instead of civilizations.

Scientists
Fritz ZwickyRashid Alievich SunyaevJames JeansVera RubinSubrahmanyan ChandrasekharAdam Riess
Concepts
neural network galaxy mapping graph neural network galaxy growth mechanisms generative model granger causality Graphs genetic algorithm Large Language Models supercomputer simulation chemical galactic archaeology dark matter deficient dwarf galaxies galactic evolution processes star formation rate stellar model random forest stellar population Generative Adversarial Networks molecular property prediction machine learning materials illustristng