The Rise of AI in Astrophysical Simulations: A Game-Changer at RIKEN
At the RIKEN Center for Interdisciplinary Theoretical and Mathematical Sciences (iTHEMS) in Japan, researchers are embarking on a groundbreaking venture where artificial intelligence (AI) squares off against traditional supercomputing methods. This initiative has led to significant advancements in simulating galaxy evolution, unlocking potential insights into the origins of the Milky Way and the very elements that underpin life as we know it.
Collaboration at the Cutting Edge of Science
The research was spearheaded by Keiya Hirashima, a Postdoctoral Researcher at iTHEMS and the Flatiron Institute’s Center for Computational Astrophysics. He was joined by an international team of experts from prominent institutions, including the Max Planck Institute for Astrophysics, the University of Tokyo, and New York University, among others. This diverse collaboration underscores the importance of teamwork in tackling complex scientific problems.
The Complex Challenge of Simulating Supernovae
A critical focal point of this research is understanding the role of supernovae in galaxy formation. Given that these cosmic events are infrequent and difficult to study, scientists traditionally rely on numerical simulations, which are inherently complex. These simulations must incorporate various cosmological forces and maintain high temporal resolution to capture the rapid dynamics of supernovae—from their core collapse to their remnants, a process that unfolds over a few months to a few thousand years.
Traditional Simulations: Limitations and Bottlenecks
Conventional numerical simulations typically operate on timescales that are about 1,000 times slower than reality, making it challenging to achieve the necessary detail in modeling smaller galaxies. Consequently, high-fidelity simulations take 1-2 years to complete, often yielding results only for smaller systems. This inefficiency forms a significant bottleneck in astrophysical research.
Introducing AI into Astrophysical Simulations
To overcome these obstacles, Hirashima’s team opted to integrate AI into their simulation framework. They built upon the ASURA code, which employs a combination of N-body and Smoothed Particle Hydrodynamics (SPH) methods to mimic galaxy formation. By also utilizing the Framework for Developing Particle Simulator (FBPS) code for chemical processes, along with a machine learning model developed by Preferred Networks Inc., they created the novel ASURA-FBPS-ML model.
Enhanced Efficiency with AI
This new AI-enhanced model significantly accelerates computational timelines. As Hirashima notes, “When we use our AI model, the simulation is about four times faster than a standard numerical simulation. This corresponds to a reduction of several months to half a year’s worth of computation time.” Remarkably, the AI-assisted simulation was able to replicate the dynamics crucial for galaxy evolution and matter cycles, including processes like star formation and galaxy outflows.
Training the AI: A Data-Driven Approach
The AI was trained using data from 300 simulations centered on an isolated supernova within a molecular cloud that weighs a million times more than our Sun. This process culminated in a model proficient in predicting critical parameters such as gas density, temperature, and 3D velocities during the early stages of supernova shell expansion—a phase that spans roughly 100,000 years.
Promising Results and Future Directions
The outcomes of the ASURA-FBPS-ML model indicate that it yields comparable galactic structures and a star formation history in a fraction of the time it takes traditional simulations. This exciting breakthrough opens doors to further applications, such as high-resolution star-by-star analyses of larger galaxies, including our own Milky Way.
Implications for Understanding the Universe
With the potential to model the evolution of the Universe since the Big Bang approximately 14 billion years ago, this AI-enhanced framework could illuminate the origins of our Solar System and the elemental building blocks of life. The research team is actively exploring these possibilities, with ambitions to enhance our understanding of complex astrophysical processes.
The findings of this groundbreaking research are detailed in a recent publication in The Astrophysical Journal, setting the stage for a new era in astrophysics where AI plays a pivotal role in exploring the cosmos.

