Analytical and Laboratory

Massive Dark Matter Detector Project Breaks Ground in South Dakota

12 February 2018

The LUX-ZEPLIN (LZ) project is now under construction in Lead, South Dakota. The project looks to build a dark matter detector utilizing seven tonnes of liquid xenon, all located nearly one mile underground.

LUX-ZEPLIN is the second-generation effort of the original large underground xenon (LUX) experiment undertaken to detect weakly interacting massive particles (WIMPs). WIMPs are hypothetical particles believed to constitute dark matter, which scientists believe makes up 80 percent or more of the known universe.

According to Sanford Underground Research Facility, renovations to Davis Cavern began on January 29 to accommodate the new LZ detector. Davis Cavern held the original LUX detector from 2012-2016.

The original LUX detector is a time projection chamber using 370 kg of liquid xenon. Interactions in the xenon generate 175 nm photons comprising the first signal, which is then detected by two arrays of 61 photomultiplier tubes (PMT). Electrons also produced by the xenon interactions eventually generate electroluminescent photons detected as the second signal. The time between the two signals is used to analyze particle behavior and possibly detect WIMPs.

The LUX-ZEPLIN dark matter detector. Source: LZ / Berkeley LabThe LUX-ZEPLIN dark matter detector. Source: LZ / Berkeley LabThe LUX-ZEPLIN detector is similar in principle to the original LUX detector, but is significantly larger. The new detector uses seven metric tons of liquid xenon, nearly 19 times more than the original LUX. It also employs 494 primary photomultiplier tubes and an additional 251 PMTs.

Both detectors are designed to operate deep underground because the layers of earth above the devices shield them from cosmic rays and radiations, which may interact with the xenon. They are also surrounded by a water tank for extra shielding.

The original LUX detector ran from October 2014 to May 2016 at four times its initial sensitivity but detected no signs of WIMPs. Data from LUX has helped scientists narrow some existing theories about WIMPs, however. The LUX-ZEPLIN’s larger xenon capacity and large amount of PMTs should give it enhanced sensitivity compared to the original detector.

The LZ project is a collaboration between 250 scientists from 37 institutions in the U.S., Russia, Portugal, Korea and the U.K. It became an official U.S. Department of Energy project in early 2015 and was approved for construction in February 2017. The Department of Energy and the U.S. National Science Foundation have selected LZ as one of three Generation-2 dark matter experiments.

To contact the author of this article, email jonathan.fuller@ieeeglobalspec.com


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