8 Jul 2014 San Diego - Light from tiny galaxies more than 13 billion years ago played a larger role than previously thought in creating the conditions in the universe as we know it today, according to a new study by researchers at the Georgia Institute of Technology and the San Diego Supercomputer Center (SDSC) at the University of California, San Diego. Ultraviolet (UV) light from stars in these faint dwarf galaxies helped strip interstellar hydrogen of electrons in a process called reionization, researchers said in a paper published in the journalMonthly Notices of the Royal Astronomical Society.
The epoch of reionization began about 200 million years after the Big Bang and astrophysicists agree that it took about 800 million more years for the entire universe to become reionized. It marked the last major phase transition of gas in the universe, and it remains ionized today.
Astrophysicists aren't in agreement when it comes to determining which type of galaxies played major roles in this epoch. Most have focused on larger, more luminous galaxies. However, this latest research, based on computer simulations, indicates scientists should also focus on the smallest ones. Specifically, these new simulations show that these tiny galaxies - despite being 1000 times smaller in mass and 30 times smaller in size than the Milky Way - contributed nearly 30 percent of the UV light during this process.
Reionization experts often ignored these dwarf galaxies because they didnt think they formed stars. It was assumed that UV light from nearby galaxies was too strong and suppressed these tiny neighbours.
"It turns out they did form stars, usually in one burst, around 500 million years after the Big Bang", stated John H. Wise, a Georgia Tech assistant professor in the School of Physics who led the study. "The galaxies were small, but so plentiful that they contributed a significant fraction of UV light in the reionization process."
The team's simulations modeled the flow of UV stellar light through the gas within galaxies as they formed. They found that the fraction of ionizing photons escaping into intergalactic space was 50 percent in small (more than 10 million solar masses) halos, or spheroidal collections of dark matter which is the site of galaxy formation. It was only 5 percent in larger halos (300 million solar masses). This elevated fraction, combined with their high abundance, is exactly the reason why the faintest galaxies play an integral role during reionization.
"It's very hard for UV light to escape galaxies because of the dense gas that fills them", stated John H. Wise. "In small galaxies, there's less gas between stars, making it easier for UV light to escape because it isn't absorbed as quickly. Plus, supernova explosions can open up channels more easily in these tiny galaxies in which UV light can escape."
The team's simulation results provide a gradual timeline that tracks the progress of reionization over hundreds of millions of years. About 300 million years after the Big Bang, the universe was 20 percent ionized. It was 50 percent at 550 million years. The universe was fully ionized at 860 million years after its creation.
"That such small galaxies could contribute so much to reionization is a real surprise", stated Michael Norman, distinguished professor of physics at UC San Diego and one of the co-authors of the paper.
"Once again, the supercomputer is teaching us something new and unexpected, something that will need to be factored into future studies of reionization", stated Michael Norman, who also is the director of SDSC, an Organized Research Unit of UC San Diego.
The term 'reionized' is used because the universe was ionized immediately after the fiery Big Bang. During that time, ordinary matter consisted mostly of hydrogen atoms with positively charged protons stripped of their negatively charged electrons. Eventually, the universe cooled enough for electrons and protons to combine and form neutral hydrogen. They didn't give off any optical or UV light. Without the light, astrophysicists aren't able to see traces of how the cosmos evolved during these Dark Ages using conventional telescopes. The light returned when reionization began, allowing experts such as John H. Wise to pinpoint the youngest galaxies and study their features.
The research team expects to learn more about these faint galaxies when the next generation of telescopes is operational. For example, NASA's James Webb Space Telescope, scheduled to launch in 2018, will be able to see them.
In addition to John H. Wise and Michael Norman, the research team included Vasiliy G. Demchenko and Martin T. Halicek, Center for Relativistic Astrophysics, Georgia Institute of Technology; Matthew J. Turk, Department of Astronomy, Columbia University; Tom Abel, Kavli Institute for Particle Astrophysics and Cosmology, Stanford University; and Britton D. Smith, Institute of Astronomy, University of Edinburgh. The research was supported by the National Science Foundation (NSF) under award numbers AST 1211626, AST 1333360, and AST 1109243.
Videos from the simulations, done using SDSC's Trestles supercomputer and additional systems at NASA, are at https://www.youtube.com/watch?v=0F_5XXU6nH0 and https://www.youtube.com/watch?v=YNQphDLn0Rc .