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Virtual Universes Reveal the Cosmos with Greater Precision ⚡ экспресс

Original: "Field-level multi-tracers simulation-based inference of cosmological parameters from 3D maps"
arXiv:2605.26210 · 2026-05-25 · CC BY 4.0 · ⏱ 1 min · Cosmology General Relativity
A new approach comparing real and virtual maps of the cosmos enables more precise measurement of the Universe's elusive properties.
Abstract

To maximize cosmological information extraction from large-scale structure data, the authors propose a Simulation-Based Inference (SBI) pipeline. Neural network emulators, trained on full hydrodynamic simulations, rapidly generate maps of galaxy positions and neutral hydrogen (HI) intensity from approximate dark matter simulations. Combined with neural posterior estimation, this framework constrains Ωm and σ8 while marginalizing over astrophysical uncertainties. Comparing inference using power spectra versus field-level data (2D and 3D maps) reveals that moving from summary statistics to the full field improves the figure of merit by roughly a factor of 3, with 3D maps yielding the most accurate and well-calibrated posteriors. Jointly analyzing galaxy and HI data tightens constraints by a factor of 2–7 over single tracers, depending on configuration.

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Astronomers build maps of galaxies and listen to the radio whisper of neutral hydrogen. The signal is so faint that even a working TV would drown it out, but sensitive antennas pick it up from the depths of the Universe. To understand how much dark matter it contains and how fast it's expanding—a process driven by the expansion of space—scientists have turned to computer simulations.

The method is like a chef who, by trying different combinations of ingredients, recreates an unknown recipe. Thousands of virtual universes are launched with varying amounts of dark matter and other parameters, until one produces a map indistinguishable from the real thing.

Previously, maps yielded only averaged metrics, as if judging a soup's taste only by its broth. The new approach captures all the nuances—both the clumpiness of galaxy clusters and the delicate filaments between them.
The method is accurate even if we don't know how galaxies are born. It adapts to uncertainties, like an experienced chef working with available ingredients.

Applying the approach simultaneously to galaxy and hydrogen maps improved accuracy 2–7 times. 3D maps add another threefold gain. This will allow us to peer into the early Universe and see if dark matter holds any new surprises.

🎯 The signal from neutral hydrogen comes at a wavelength of 21 centimeters. It's so faint that a working TV could drown it out, but astronomers capture it with sensitive antennas.

🎬 In the iconic Matrix trilogy, reality turned out to be a computer simulation. In this work, scientists, on the contrary, use simulations to uncover the true nature of our world.

Scientists
Adam RiessBrian SchmidtEdwin HubbleGeorges LemaîtreMaarten SchmidtSaul Perlmutter
Tags
galaxy hydrogen dark matter expansion of the universe
Laws
Hubble's lawgravitational lensingCoulomb's lawRydberg formulavirial theoremBalmer formula
Original: arXiv:2605.26210 · CC BY 4.0 · bridge42worlds