See and hear galaxies evolve from the dawn of the universe

The most realistic picture yet of how galaxies formed and then evolved from the beginning of time has been revealed in a suite of new and unique audiovisual simulations. These data, accepted for publication in the Monthly Notices of the Royal Astronomical Society, show that the standard cosmological model can successfully explain the observed growth of galaxies, from the first billion years after the Big Bang to the present day, when key physics is included.

Unlike earlier simulations, the COLIBRE “virtual universes” model the cold gas and cosmic dust inside galaxies—the raw materials from which stars form and which strongly affect how galaxies look in telescopes.

By including these previously missing ingredients and using far more computing power than ever before, the simulations successfully reproduce real galaxies, both in the present-day universe and in the early universe as seen by the James Webb Space Telescope (JWST).

“Much of the gas inside real galaxies is cold and dusty, but most previous large simulations had to ignore this,” said project leader Professor Joop Schaye, of Leiden University. “With COLIBRE, we finally bring these essential components into the picture.”

The results show that our standard model of the universe can explain galaxy formation more accurately than previously thought, while also opening up powerful new ways to compare theory with observations and to explore a virtual universe through visuals, sound, and interactive tools.

Digital cold gas and dust grains

According to the international team of researchers, their COLIBRE simulations break new ground in several ways. Earlier simulations artificially prevented gas inside galaxies from cooling below about 10,000 degrees Fahrenheit—hotter than the surface of the sun—because modeling colder gas was too complex. Yet, observations show that stars form in cold gas. COLIBRE includes the additional physical and chemical processes needed to model this cold interstellar gas directly.

COLIBRE also simulates small dust grains, which can greatly influence galactic gas. These solid particles can help hydrogen molecules to form, which dominate the cold gas content of galaxies. The dust also shields gas from harsh ultraviolet radiation and strongly affects how galaxies appear in telescopes. Dust absorbs ultraviolet and optical light from stars and re-emits it in the infrared, shaping many astronomical observations. By modeling dust directly, COLIBRE opens new ways to compare simulations with real data.

Thanks to advances in algorithms and supercomputing, COLIBRE uses up to 20 times more resolution elements than earlier simulations, allowing larger volumes to be simulated in greater detail and with better statistics.

A new laboratory

COLIBRE demonstrates that realistic treatments of cold gas, dust, and outflows driven by stars and black holes are crucial for understanding galaxy evolution, the researchers say. It provides a powerful new laboratory for testing theories, interpreting observations, and creating “virtual observations” to check how astronomers analyze real data.

The findings also show that the standard cosmological model remains consistent with observations of galaxy evolution, including some that were thought to be challenging, such as the masses of galaxies in the early universe.

“Some early JWST results were thought to challenge the standard cosmological model,” said Dr. Evgenii Chaikin, of Leiden University, lead author of several accompanying COLIBRE papers and co-author of the main study. “COLIBRE shows that, once key physical processes are represented more realistically, the model is consistent with what we see.”

Still, not everything has been explained yet. The enigmatic “Little Red Dots” discovered by JWST, possibly the seeds of supermassive black holes, are not predicted by COLIBRE, which assumes such seeds already exist. Modeling their formation will require even higher resolution simulations and new physics, pointing the way for future work.

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The simulations were run using the SWIFT simulation code on the COSMA8 supercomputer at the Institute for Computational Cosmology at Durham University, which is hosted on behalf of the DiRAC national facility in the UK. The largest simulation required 72 million CPU hours, and the full model took nearly 10 years to develop by an international team spanning Europe, Australia, and the United States.

Carlos Frenk, Ogden Professor of Fundamental Physics at the Institute for Computational Cosmology at Durham University, and a core member of the COLIBRE team said, “It is exhilarating to see ‘galaxies’ come out of our computer that look indistinguishable from the real thing and share many of the properties that astronomers measure in real data such as their number, luminosities, colors and sizes.

“I like to tease my observer colleagues by asking ‘which galaxy catalog do you think these images came from?'”

He added, “What is most remarkable is that we are able to produce this synthetic universe purely by solving the relevant equations of physics in the expanding universe.”

The scientists point out that it will take years to analyze the data that has already been produced. Most simulations were completed in 2025, although some of the simulations with the highest resolution are still running and are expected to finish after the summer.

A universe you can see and hear

Beyond traditional data products, the team has developed new ways to explore the simulations. This includes “sonified videos,” where sound encodes additional physical information, as well as interactive maps that allow users to explore the virtual universes.

“We’re excited not just about the science, but also about creating new ways to explore it,” said Dr. James Trayford, of the University of Portsmouth, who led the development of COLIBRE’s dust model and the sonification of its visualizations.

“These tools could provide new insights, make our field more accessible, and help us build intuition for how galaxies grow and evolve.”