Derenzo said the new detector would be similar in construction to another experiment, called the Super Cryogenic Dark Matter Search (SuperCDMS) which uses low-temperature solid state detectors the size of hockey pucks. The original experiment was done in the Soudan Underground Laboratory, a former iron mine in Minnesota, and a larger experiment is being built in the deeper SNOLAB in Sudbury, Canada. It looks for dark matter in a type of interaction known as a nuclear recoil.
But the proposed new detector would be able to look for much smaller than WIMPs.
“SuperCDMS is sensitive to nuclear recoils from dark matter in the energy range above the mass of the proton,” Derenzon said. “Gallium arsenide is sensitive to electron recoils in the range below the mass of the proton. These
approaches are complementary since there may be dark matter particles of different masses.”
RELATED: This Is the Most Detailed Simulation of the Universe
While astronomers and physicist don’t know what dark matter is, they can measure the effect of its gravity on stars and galaxies. In the 1930s, astronomer Fritz Zwicky first noticed that the motion of galaxies he was studying in the Coma cluster couldn’t be accounted for by the gravity from visible matter of stars, gas, and dust. Then in the 1970s, Vera Rubin and her colleagues determined there wasn't enough "normal" mass present in the galaxies they were studying to explain their rate of rotation. This presented a problem, as either our understanding of gravity was flawed, or there was about five times more mass in the galaxies than astronomers could see.
Normal matter accounts for only about 5 percent of matter in the universe, whereas dark matter constitutes more than 25 percent. The remaining 70 percent is known as dark energy, which, like dark matter, has not been directly observed by researchers.
Astronomers are convinced, however, that dark matter — as well as dark energy — exists and have tried to observe them in several ways, including in underground laboratories and supercolliders such as CERN in Switzerland.
To build any type of dark matter detector, researchers have had to make some assumptions about the nature of the dark matter. Based on a number of theoretical studies, WIMPs were thought to be the likely main constituent of dark matter.
Therefore, most detectors have been built to detect particles the size of WIMPs, thought to weigh more than 100 times the mass of a proton.
RELATED: Gravitational Waves From Colliding Neutron Stars Detected for the First Time
Derenzo and his colleague wrote that despite overwhelming evidence for dark matter, recent large-scale experiments designed to detect nuclear recoils from dark matter particles with masses of WIMPs have not yet seen a definitive signal. This has motivated designs for experiments that search for dark matter particles in a different size range.
The GaAs crystal detector would operate near absolute zero, or nearly minus 460 degrees Fahrenheit. This new design iS the first time gallium arsenide would be used as a cryogenic scintillation detector. The detector will be combined with a cryogenic photodetector, which can detect light at very low temperatures. Derenzo said the new detector could be “a workhorse useful in the search for dark matter in a largely unexplored mass range.”
Work toward constructing the detector is ongoing, Derenzo said.
“The next steps involve a scale-up from small (10 millimeter) to larger (10 centimeter) GaAs crystals and to large (10 centimeter) TES photodetectors,” he said. “There are no fundamental technical problems and the scale-up costs should be similar to SuperCDMS.”
The cost for SuperCDMS is about $32 million. A much bigger but similar experiment called the Large Underground Xenon dark matter experiment (LUX) comes in at a cost of $55 million.
“It’s hard to imagine a better material for searching in this particular mass range,” Derenzo said. “It ticks all of the boxes. We are always worried about a ‘Gotcha!’ or showstopper. But I have tried to think of some way this detector material can fail and I can’t.”