The faintest and smallest galaxies played a bigger role than previously thought in shining ultraviolet light in the early universe, experts now say.
That UV light was essential to reionization, a process that began about 200 million years after the Big Bang. Astrophysicists agree that it took about 800 million more 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 of reionization. Most have focused on large galaxies.
However, a new theory by researchers at the Georgia Institute of Technology and the San Diego Supercomputer Center indicates scientists should also focus on the smallest. The findings are reported in a paper published in the Monthly Notices of the Royal Astronomical Society.
The researchers used computer simulations to demonstrate the faintest and smallest galaxies in the early universe were essential. 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.
A view of the entire simulation volume showing the large scale structure of the gas, which is distributed in filaments and clumps. The red regions are heated by UV light coming from the galaxies, highlighted in white. These galaxies are over 1000 times less massive than the Milky Way and contributed nearly one-third of the UV light during re-ionisation. The field of view of this image is 400,000 light years across, when the universe was only 700 million years old. (John Wise)
What Is Reionization?
The term reionized is used because the universe was ionized immediately after the fiery Big Bang. During that time, ordinary matter consisted 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 to pinpoint the youngest galaxies and study their features.
Small but Plentiful
Reionization experts often ignored dwarf galaxies because they didn’t think they formed stars. It is assumed that UV light from nearby galaxies was too strong and suppressed these tiny neighbors.
“It turns out they did form stars, usually in one burst, around 500 million years after the Big Bang,” says John 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. 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,” says 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.”
‘A Real Surprise’
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,” says Michael Norman, a physics professor 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.”
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.
The National Science Foundation supported the research.
Source: Georgia Tech. Republished from Futurity.org under Creative Commons License 3.0.
