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Virtual universe machine

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  • Computer simulations help scientists study the evolution of galaxies over time
  • Generating millions of universes on a supercomputer lets scientists compare theories
  • Findings challenge fundamental ideas about the role of dark matter and the birth of stars

How do galaxies such as our Milky Way come into existence? How do they grow and change over time?

The science behind galaxy formation has remained a puzzle for decades, but a University of Arizona (UA)-led team of scientists is one step closer to finding answers thanks to supercomputer simulations.

<strong>Universe machine.</strong> Scientists generated millions of different universes on a supercomputer, each of which obeyed different physical theories for how galaxies should form. Courtesy NASA, ESA, and J. Lotz and HFF Team/STScI. Observing real galaxies in space can only provide snapshots in time, so researchers who want to study how galaxies evolve over billions of years have to revert to computer simulations.

Traditionally, astronomers have used this approach to invent and test new theories of galaxy formation, one-by-one. Peter Behroozi, of the UA Steward Observatory, and his team overcame this hurdle by generating millions of different universes on a supercomputer, each of which obeyed different physical theories for how galaxies should form.

The findings challenge fundamental ideas about the role dark matter plays in galaxy formation, how galaxies evolve over time, and how they give birth to stars.

"On the computer, we can create many different universes and compare them to the actual one, and that lets us infer which rules lead to the one we see," said Behroozi.

The study is the first to create self-consistent universes that are such exact replicas of the real one. The computer simulations each represent a sizeable chunk of the actual cosmos, containing 12 million galaxies and spanning the time from 400 million years after the Big Bang to the present day.

Each "Ex-Machina" universe was put through a series of tests to evaluate how similar galaxies appeared in the generated universe compared to the true universe. The universes most similar to our own all had similar underlying physical rules, demonstrating a powerful new approach for studying galaxy formation.

<strong>A supermassive black hole</strong> at the center of an ellipical galaxy may stifle the formation of new stars. Courtesy NASA/JPL-Caltech.The results from the "UniverseMachine," as the authors call their approach, have helped resolve the long-standing paradox of why galaxies cease to form new stars even when they retain plenty of hydrogen gas, the raw material from which stars are forged.

Commonly held ideas about how galaxies form stars involve a complex interplay between cold gas collapsing under the effect of gravity into dense pockets giving rise to stars, while other processes counteract star formation. 

For example, it is thought that most galaxies harbor supermassive black holes in their centers. Matter falling into these black holes radiates tremendous energies, acting as cosmic blowtorches that prevent gas from cooling down enough to collapse into stellar nurseries.

Dark matter, too, plays a big role, as it provides for most of the gravitational force acting on the visible matter in a galaxy, pulling in cold gas from the galaxy's surroundings and heating it up in the process.

"As we go back earlier and earlier in the universe, we would expect the dark matter to be denser, and therefore the gas to be getting hotter and hotter. This is bad for star formation, so we had thought that many galaxies in the early universe should have stopped forming stars a long time ago," Behroozi said. "But we found the opposite: galaxies of a given size were more likely to form stars at a higher rate, contrary to the expectation."

In order to match observations of actual galaxies, Behroozi explained, his team had to create virtual universes in which the opposite was the case – universes in which galaxies kept churning out stars for much longer.

According to Behroozi, creating mock universes of unprecedented complexity required an entirely new approach that was not limited by computing power and memory, and provided enough resolution to span the scales from the "small" – individual objects such as supernovae – to a sizeable chunk of the observable universe.

<strong>The Ocelote supercomputer</strong> at the University of Arizona helped researchers generate more than 8 million universes. Courtesy Daniel Stolte/UANews."Simulating a single galaxy requires 10 to the 48th computing operations," he explained. "All computers on Earth combined could not do this in a hundred years. So to just simulate a single galaxy, let alone 12 million, we had to do this differently."

In addition to utilizing computing resources at NASA Ames Research Center and the Leibniz Supercomputing Centre in Germany, the team used the Ocelote supercomputer at the UA High Performance Computing cluster. Two thousand processors crunched the data simultaneously over three weeks. Over the course of the research project, Behroozi and his colleagues generated more than 8 million universes.

"We took the past 20 years of astronomical observations and compared them to the millions of mock universes we generated," Behroozi explained. "We pieced together thousands of pieces of information to see which ones matched. Did the universe we created look right? If not, we'd go back and make modifications, and check again."

Behroozi and his colleagues plan to expand the UniverseMachine to include the morphology of individual galaxies and how their shapes evolve over time.

Read the original article on UA's site.

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