Sciences. – Recording simulations of the formation of large-scale cosmic structures

Madrid, 3 (Europe Press)

New simulations of the formation of cosmic structures are able to accurately reproduce the complex dynamics of the elusive neutrinos left in the universe as a result of the Big Bang.

The study was published in SC ’21: Proceedings of the International Conference on High-Performance Computing, Networks, Storage and Analysis, by researchers from the University of Tsukuba, Kyoto University and the University of Tokyo.

Neutrinos are much lighter than all other known particles, but their exact mass remains a mystery. Measuring this mass can help scientists develop theories beyond the Standard Model of particle physics and test explanations for how the universe evolved. A promising method for determining this mass is to study its effect on the formation of large-scale structures using simulations and compare the results with observations. But this simulation has to be very accurate.

“Standard simulations use techniques known as particle-based N-body methods, which have two main drawbacks when it comes to massive neutrinos,” explains Dr. Naoki Yoshida, principal investigator at the university’s Kavli Institute of Physics and Mathematics. Tokyo. “First, simulation results are subject to random fluctuations called firing noise. Second, these particle-based methods cannot accurately produce collision-free damping, a fundamental process in which fast-moving neutrinos suppress structure growth in the universe.”

To avoid these problems, researchers have followed the dynamics of massive neutrinos by directly solving a central equation in plasma physics known as the Vlasov equation. In contrast to previous studies, they solved this equation in a full six-dimensional phase space, which means that all six dimensions associated with space and velocity were considered. The team combined the Vlasov simulation with an N-body simulation based on particles of cold dark matter, the main component of matter in the universe. They ran their hybrid simulations on a Fugaku supercomputer at the RIKEN Center for Computer Science.

“Our largest simulation consistently combines Vlasov simulations on 400 trillion grids with calculations of 330 billion objects, accurately reproducing the complex dynamics of cosmic neutrinos,” says Professor Koji Yoshikawa, lead author of the study. “In addition, the resolution time for our simulations is significantly shorter than that of the larger N-body simulation, and performance metrics are very good with up to 147,456 nodes (7 million CPUs) on Fugaku.”

In addition to helping determine the mass of neutrinos, the researchers suggest that their scheme could be used to study, for example, phenomena involving electrostatic and magnetic plasmas and gravitational systems.