Brown University is taking part in the
Hydrogen Epoch of Reionization Array (HERA) collaborative experiment, which
recently received $9.5 million in funding from the National Science Foundation
to expand the capabilities of its telescope.
The project is looking back more than 13.5
billion years ago to the time when the first stars began producing light. They
are looking for signals of the hydrogen ionization process, which created the
ionized hydrogen found in the universe today, to better understand what the
first stars and galaxies were like.
“We’re looking back to the time when ionization was still happening,” Brown Assistant Professor of Physics Jonathon Pober, who is a member of
the HERA science team, said. “Neutral hydrogen emits radiation at a wavelength of 21
centimeters, and that’s the signal we’re tracking. As reionization happens, and
these bubbles of ionized hydrogen start growing, the 21-centimeter signal of
neutral hydrogen decreases. So we’re effectively looking for the disappearance
of this signal.”
The array itself currently comprises 19
radio dishes located near Carnarvon, South Africa, but the new funding from the
National Science Foundation will allow the experiment to install a further 221
dishes by 2018. Brown’s role in the experiment, which is led by the University
of California at Berkeley, is to confirm the signal once found.
“The signal we’re
looking for is really faint, so we need a bevy of tools for discriminating that
signal from all the other stuff we might be seeing,” Pober said. “When we
detect a signal, and I truly hope we will, it’s going to take a lot of
convincing — both internally within the experiment and externally — that the
signal is real, so that’s what we’ll be focusing on at Brown. And if we can
confirm that signal, we’ll be documenting a cornerstone event in cosmic
history.”
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