July 10, 2025
press release
Physics/Astronomics
Computing/Mathematics
In the first study of this kind, researchers led by Hiroshima Keiya of the Riken Center in Japan's Interdisciplinary Theory and Mathematical Sciences (ITHEMS), as well as colleagues from the Max Planck Institute for Astrophysics (MPA) and Flatiron Institute, have used galaxies. Combined with the supernova explosion. This approach helps us understand the origins of our own galaxies, especially the essential elements of life in the Milky Way.
Understanding how galaxies form is a central issue for astrophysicists. We know that powerful events like supernovae can promote the evolution of galaxies, but we can't look to the night sky and see it happen. Scientists rely on numerical simulations based on a large amount of data collected from telescopes and other devices measuring aspects of interstellar space. Simulations need to explain other complex aspects of gravity and fluid mechanics, as well as astrophysical chemistry.
In addition to this, they must have a high temporal resolution. In other words, the time between each 3D snapshot of an evolving galaxy must be small enough to avoid missing important events. For example, capturing the early stages of supernova shell expansion requires a timescale of several hundred years, which is 1000 times less than a typical simulation of interstellar space. In fact, a typical supercomputer takes 1-2 years to perform simulations of relatively small galaxies with appropriate time resolution.
Overcoming this time step bottleneck was the main goal of the new research. By incorporating AI into a data-driven model, the research group was able to match the outputs of previously modeled dwarf galaxies, but they got results more quickly. “When using AI models, simulations are about four times faster than standard numerical simulations,” says Hirashima. “This corresponds to reducing computational time from several months to six months. Critical, our AI-assisted simulations were able to replicate the dynamics that are important for capturing galaxy evolution and material cycles, such as star formation and galaxy outflow.”
Like most machine learning models, researchers' new models are trained using one dataset to allow them to predict results based on the new dataset. In this case, the model incorporates a programmed neural network and was trained on 300 simulations of isolated supernovas of molecular clouds, carrying a large amount of one million suns. After training, the model was able to predict gas density, temperature, and 3D speeds 100,000 years after the supernova explosion. Compared to direct numerical simulations, such as those performed by supercomputers, the new model produced similar structures and star formation history, but the calculation took four times longer.
According to Hiroshima, “Our AI-assisted framework allows for high-resolution Starby Star simulations of heavy galaxies such as the Milky Way, with the aim of predicting the origins of the solar system and the essential elements of the birth of life.”
Currently, the lab is using a new framework to perform Milky Way-sized galaxy simulations.
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Hiroshima Keiya, a special postdoctoral researcher
Department of Fundamental Mathematics Science, Riken Center for Interdisciplinary Theory and Mathematical Sciences (ITHEMS)
Adam Phillips
Riken Communications Division
Email: Adam.Phillips [at] riken.jp
A simulated galaxy 200 million years later. Simulations appear to be very similar to machine learning AI models, but the AI models run 4 times faster, completing large-scale simulations in months rather than years.
