Small clip for simulation of Thesan. See the video in the article below.
Named after the dawn goddess, Thesan’s simulations of the first billion years help explain how radiation shaped the early universe.
It all started about 13.8 billion years ago with a huge cosmic “explosion” that suddenly and amazingly created the universe. Soon, the infant universe cooled dramatically and became completely dark.
Then, within a few hundred million years after[{” attribute=””>Big Bang, the universe woke up, as gravity gathered matter into the first stars and galaxies. Light from these first stars turned the surrounding gas into a hot, ionized plasma — a crucial transformation known as cosmic reionization that propelled the universe into the complex structure that we see today.
Now, scientists can get a detailed view of how the universe may have unfolded during this pivotal period with a new simulation, known as Thesan, developed by scientists at MIT, Harvard University, and the Max Planck Institute for Astrophysics.
Named after the Etruscan goddess of the dawn, Thesan is designed to simulate the “cosmic dawn,” and specifically cosmic reionization, a period which has been challenging to reconstruct, as it involves immensely complicated, chaotic interactions, including those between gravity, gas, and radiation.
The Thesan simulation resolves these interactions with the highest detail and over the largest volume of any previous simulation. It does so by combining a realistic model of galaxy formation with a new algorithm that tracks how light interacts with gas, along with a model for cosmic dust.
Evolution of simulated properties in the main Thesan run. Time progresses from left to right. The dark matter (top panel) collapse in the cosmic web structure, composed of clumps (haloes) connected by filaments, and the gas (second panel from the top) follows, collapsing to create galaxies. These produce ionizing photons that drive cosmic reionization (third panel from the top), heating up the gas in the process (bottom panel). Credit: Courtesy of THESAN Simulations
With Thesan, the researchers can simulate a cubic volume of the universe spanning 300 million light years across. They run the simulation forward in time to track the first appearance and evolution of hundreds of thousands of galaxies within this space, beginning around 400,000 years after the Big Bang, and through the first billion years.
So far, the simulations align with what few observations astronomers have of the early universe. As more observations are made of this period, for instance with the newly launched James Webb Space Telescope, Thesan may help to place such observations in cosmic context.
For now, the simulations are starting to shed light on certain processes, such as how far light can travel in the early universe, and which galaxies were responsible for reionization.
“Thesan acts as a bridge to the early universe,” says Aaron Smith, a NASA Einstein Fellow in MIT’s Kavli Institute for Astrophysics and Space Research. “It is intended to serve as an ideal simulation counterpart for upcoming observational facilities, which are poised to fundamentally alter our understanding of the cosmos.”
Smith and Mark Vogelsberger, associate professor of physics at MIT, Rahul Kannan of the Harvard-Smithsonian Center for Astrophysics, and Enrico Garaldi at Max Planck have introduced the Thesan simulation through three papers, the third published on March 24, 2022, in the Monthly Notices of the Royal Astronomical Society.
Follow the light
In the earliest stages of cosmic reionization, the universe was a dark and homogenous space. For physicists, the cosmic evolution during these early “dark ages” is relatively simple to calculate.
“In principle you could work this out with pen and paper,” Smith says. “But at some point gravity starts to pull and collapse matter together, at first slowly, but then so quickly that calculations become too complicated, and we have to do a full simulation.”
To fully simulate cosmic reionization, the team sought to include as many major ingredients of the early universe as possible. They started off with a successful model of galaxy formation that their groups previously developed, called Illustris-TNG, which has been shown to accurately simulate the properties and populations of evolving galaxies. They then developed a new code to incorporate how the light from galaxies and stars interact with and reionize the surrounding gas — an extremely complex process that other simulations have not been able to accurately reproduce at large scale.
“Thesan follows how the light from these first galaxies interacts with the gas over the first billion years and transforms the universe from neutral to ionized,” Kannan says. “This way, we automatically follow the reionization process as it unfolds.”
Finally, the team included a preliminary model of cosmic dust — another feature that is unique to such simulations of the early universe. This early model aims to describe how tiny grains of material influence the formation of galaxies in the early, sparse universe.
This simulation of gas evolution and radiation shows an embodiment of neutral hydrogen gas. The colors represent intensity and brightness, revealing the incomplete reionization structure within a network of high-density neutral gas filaments.
cosmic bridge
With the simulation components in place, the team determined its initial conditions for about 400,000 years after the Big Bang, based on precise measurements of the Big Bang’s remnant light. They then developed these conditions forward in time to simulate a swath of the universe, using the SuperMUC-NG machine – one of the world’s largest supercomputers – which simultaneously harnessed 60,000 computer cores to perform Thesan calculations on the equivalent of 30 million CPUs. . an hour (an effort that would have taken 3,500 years to run on a single desktop).
The simulations produced the most detailed view of cosmic reionization, across the largest volume of space, of any simulation in existence. While some simulations run over large distances, they do so at a relatively low resolution, while other, more detailed simulations do not span large sizes.
“We traverse between these two approaches: we have high volume and high precision,” emphasizes Vogelsberger.
Early analyzes of the simulations indicate that at the end of cosmic reionization, the distance that enables light to travel has increased significantly more than scientists previously assumed.
“Thesan found that light does not travel great distances in the early universe,” Canan says. “In fact, this distance is very small, and it only becomes large at the end of reionization, increasing by 10 times in just a few hundred million years.”
Researchers are also seeing hints about the type of galaxies responsible for reionization. The galaxy’s mass appears to influence reionization, although the team says more observations, taken by James Webb and other observatories, will help identify these dominant galaxies.
“There are a lot of moving parts in [modeling cosmic reionization]’, concludes Vogelsberger. “When we can put all of this together in some kind of machine and start to run it and result in a dynamic universe, that for all of us is a very rewarding moment.”
Reference: “This Project: Lyman-A Emission and Transfer during the Reionization Era” by A Smith, R. Cannan, E. Garaldi, M. Vogelsberger, R. Buckmore, in Sprinkle and L. Hernquist, March 24, 2022 Available here Monthly Notices of the Royal Astronomical Society.
DOI: 10.1093/mnras/stac713
This research was supported in part by NASA, the National Science Foundation, and the Gauss Center for Supercomputing.