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Small buildins sit on field of ice and snow.
Photo Credit: Jeffrey Donenfeld
The ARA field camp at the South Pole is set up to deploy a station that will eventually be used to detect high-energy neutrinos.

A bigger mousetrap

New neutrino detector prototype at South Pole goes after highest energy particles

To catch the elusive subatomic particles called neutrinos is not just a matter of building a better mousetrap. You need a really, really BIG mousetrap.

Physicist Albrecht Karle External Non-U.S. government site and colleagues hope to construct a neutrino detector across more than 100 square kilometers of Antarctica’s polar plateau to capture some of the highest energy neutrinos theorized to exist – byproducts of ultra-high energy cosmic rays emitted from astronomical objects such as galaxies with supermassive black holes a billion or more light years away.

Three of 37 proposed stations in the Askaryan Radio Array (ARA) External Non-U.S. government site have been installed near the U.S. Antarctic Program’s South Pole Station External U.S. government site over the last two years. The project is still in its proof-of-concept stage, as researchers refine the design of the array and test alternative energy technologies that will be required to power ARA as it spreads away from the research station.

People hook up cables.
Photo Credit: Peter Rejcek
The ARA team, led by Albrecht Karle, second from left, hook up the cables for one of the antennas in the array.

The South Pole is already home to the world’s biggest (to date) neutrino telescope. The IceCube Neutrino Observatory External Non-U.S. government site is a detector buried within a cubic kilometer of ice. It uses vertically aligned strings of basketball-sized photomultipliers, somewhat like specially designed digital cameras, which capture an incredibly brief flash of light that is produced when a neutrino makes a rare collision in the ice. [See previous article — Stringing it together: IceCube team completes massive neutrino detector at South Pole.]

On the other hand, ARA will use radio antennae to detect equally brief radio pulses from neutrinos that originate outside the Milky Way Galaxy with energy ranges beyond what even IceCube can track.

“The full array of 37 stations would have a sensitivity or discovery potential for these highest energy neutrinos 10 times better than IceCube – and IceCube is already the best experiment even at these energies. It’s quite amazing,” said Karle, a professor in the Department of Physics External Non-U.S. government site at the University of Wisconsin-Madison External Non-U.S. government site, during an interview at the South Pole Station during the 2012-13 field season.

The array is named after Russian physicist Gurgen Askaryan who figured out that the cloud of secondary particles created in the interaction of high-energy neutrinos will create a burst of radio waves in a medium that is transparent to radio waves such as salt or ice. At high energies, these radio waves are detectable using radio antennae. 

“We use the ice as a target for interactions,” Karle explained.

Two metal towers are attached to blue building.
Photo Credit: Jeffrey Donenfeld
The IceCube Neutrino Observatory laboratory at the South Pole.

High-energy neutrinos result from violent events in the far-flung corners of the universe, such as exploding stars or by the formation of black holes. 

Physicists believe neutrinos contain clues about the origin of high-energy particles – cosmic rays – in the universe, thanks to the fact that they make a straight beeline through the universe without really changing course.

“We will have good directional resolution, so we’ll see from where these events come,” Karle said. “These neutrinos would establish a very distinct correlation to the highest energy cosmic rays. These are the ones we are trying to discover.”

How much punch do these cosmic rays carry? The particles hold about 10 million times more energy than can be produced by accelerators on Earth such as CERN’s Large Hadron Collider External Non-U.S. government site. The neutrinos are tertiary particles, created by the decay of secondary particles that result when high-energy protons from intergalactic accelerators like black holes interact with the abundant low-energy photons from the cosmic microwave background.

Karle said ARA could not only potentially establish the absolute flux of the so-called cosmogenic neutrinos, but could also determine whether the highest energy cosmic rays consist of just protons, iron nuclei, or both.

“ARA has a real prospect to answer that question and measure the cosmogenic neutrino flux,” he said.

Much work lies ahead before that happens.

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Curator: Peter Rejcek, Antarctic Support Contract | NSF Official: Winifred Reuning, Division of Polar Programs