Recreating a slice of the universe: Computational approach follows thousands of galaxies over billions of years

"We've created the full variety of galaxies we see in the local universe," said Mark Vogelsberger (CfA).

Our cosmic neighborhood is littered with majestic spiral galaxies like Andromeda, the Pinwheel, and the Whirlpool. Spirals are common, but previous simulations had trouble creating them. Instead, they produced lots of blobby galaxies clumped into balls, without the broad disks and outstretched arms of a typical spiral.

The new software, called Arepo, solves this problem. Created by Volker Springel (HITS), Arepo generates a full-fledged simulation of the universe, taking as input only the observed afterglow of the Big Bang and evolving forward in time for 14 billion years.

"We took all the advantages of previous codes and removed the disadvantages," explained Springel.

"Our simulations improve over previous ones as much as the Giant Magellan Telescope will improve upon any telescope that exists now," said Debora Sijacki (CfA).

(When completed later this decade, the Giant Magellan Telescope's 24.5-meter aperture will make it the largest telescope in the world.)

One of Arepo's key advantages is the geometry it uses. Previous simulations divided space into a bunch of cubes of fixed size and shape. Arepo uses a grid that flexes and moves in space to match the motions of the underlying gas, stars, dark matter, and dark energy.

The simulations ran on Harvard's Odyssey high-performance supercomputer, using in total 1024 processor cores. This fast machine allowed the scientists to compress 14 billion years into only a few months -- an endeavor that would have kept a desktop computer busy for hundreds of years!

The team's future goals include simulating much larger volumes of the universe at unprecedented resolution, thus creating the largest and most realistic model of the universe ever made.

The team consists of Mark Vogelsberger (CfA), Debora Sijacki (CfA), Dusan Keres (CfA/UCSD), Paul Torrey (CfA), Volker Springel (HITS), and Lars Hernquist (CfA). Their work is described in three papers accepted for publication in the Monthly Notices of the Royal Astronomical Society. Those papers can be found online at http://arxiv.org/abs/1109.1281, http://arxiv.org/abs/1109.3468, and http://arxiv.org/abs/1109.4638.