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Physicists to hunt dark matter in a former gold mine

(Credit: Matthew Kapust)

In a mine where workers once risked their lives to find gold, researchers now seek the ultimate treasure in particle physics—dark matter.

The Cage, as the elevator is called, leaves exactly at 7:30 am and slowly descends. Nearly two dozen people packed together inside wear coveralls, hard hats, and thick rubber boots to protect them from the water dripping from the timber buttressing the elevator shaft. (It’s kept wet to prevent them from drying out and rotting.) About 10 minutes later, nearly one mile down, the Cage thumps to a stop and the heavy, yellow metal doors swing open.

The men and women stream into a cavern with rough rock walls that miners once blasted with explosives in search of gold. Underfoot run the rail tracks used to wheel minecarts laden with equipment and supplies to the surface.

Further down one of the corridors, it starts to feel more civilized. Concrete walls and desks line the hallway, and fluorescent lights guide the way. There’s also a table with an espresso machine and panini maker.

Anyone venturing further must pass through a clean room where you remove your overalls, don a double layer of disposable booties, and have your possessions swabbed with alcohol.

A bit further and double doors swing open to reveal a lab. Scientists adjust equipment and take measurements. But the real center of attraction is a hulking 26-foot by 20-foot stainless steel vat in the middle of the room. In late March, the members of Brandeis University assistant professor of physics Bjoern Penning’s lab were inside it, hard at work.

Welcome to SURF

Until 2002, it was a working mine in the small town of Lead, South Dakota. Then, with state, federal, and private funding, it became the Sanford Underground Research Facility (SURF). Now, Penning and his team use the space to seek dark matter.

A mysterious, elusive substance, dark matter is thought to comprise around 85 percent of all the matter in the universe. The stuff we’re familiar with, atoms, makes up only 15 percent. We’ve known about protons, neutrons, and electrons for over 100 years, but we know next to nothing about dark matter. Evidence of its existence is overwhelming. Only by factoring in the extra mass it provides can scientists account for gravity’s effect on the arrangement and motion of galaxies.

But to date, no one’s been able to observe or detect dark matter. So Penning and his team have come to SURF to find it.

They are part of an international consortium of over 250 researchers worldwide working on what’s called the LUX-ZEPLIN (LZ) experiment. If LZ scientists succeed, it will be a revolutionary discovery that will give us a new understanding of what the cosmos is made of and how it came to be.

Penning and four lab members—senior mechanical engineer Andrei Dushkin, electrical engineer Richard Studley, graduate student Luke Korley, and postdoctoral fellow Ryan Wang—came to South Dakota to help build a dark matter detector.

Finding WIMPS

The stainless steel cauldron in which they worked is its outer shell. Dark matter is most likely made of WIMPS, weakly interacting massive particles. WIMPS are all around us, but because they’re so weak, they barely interact with other matter. This makes them “ghost particles”—they can pass right through us without registering any discernible impact.

WIMPS emit such a faint signal that they’re extremely hard to discern from all the other matter around us. The dark matter detector is designed to filter out all this background noise.

The container that scientists are building inside a former gold mine in South Dakota, in hopes of using it to detect dark matter.
The container that scientists are building inside a former gold mine in South Dakota, in hopes of using it to detect dark matter. (Credit: Matt Hoff/Lawrence Berkeley National Laboratory/Brandeis University)

The detector functions like a set of nested sieves, each one filtering out other particles so that what finally winds up in the center can only be a WIMP. Penning likes to invoke a Sherlock Holmes’ quote he’s slightly amended—”When you have eliminated all possibilities, whatever remains, however improbable, must be the truth,” the truth, in this case, being a WIMP.

The outermost sieve is actually the mountain in which the lab is buried. The dirt and rock block out by a factor of a billion the cosmic radiation particles in our atmosphere left over from the Big Bang.

Next comes the 60,000 gallons of water that will be poured into the stainless steel container. It will be ultrapure, free of contaminants that might make dark matter hard to detect, and capable of screening out gamma radiation and neutrons.

Neutrons are a particular problem since they induce a weak signal that can easily be mistaken for WIMPS. Therefore, a second sieve was added to block neutrons—10 12-foot acrylic tanks suspended in the ultrapure water and filled with liquified gadolinium and linear alkylbenzene, a common component of cleaning products. Gadolinium atoms are arranged in such a way that neutrons stick to them.

Penning’s team designed sensors to surround the acrylic tanks. At present, they are non-working test dummies made on a 3D printer and look like giant white K-Cups. They will hang on scaffolding erected along the stainless steel tank’s perimeter.

When neutrons collide with gadolinium atoms, photons are emitted. The sensors can detect these photons, ensuring everything is working as planned and no neutrons are slipping through the gadolinium barrier.

The innermost sanctum of the LZ experiment—and its pièce de résistance—is a 13-foot titanium cylinder filled with liquid xenon. It will be submerged in the ultrapure water and encircled by the acrylic tanks.

If scientists’ predictions about the behavior and composition of WIMPS are correct, when one bumps into a xenon atom, it will produce two flashes of light that only dark matter could generate. Sensors inside the titanium cylinder will probe for this signature WIMP fingerprint.

Like a ship in a bottle

During their time in South Dakota, Penning’s lab only practiced setting up the sensors they’ve built for the detector. Everything will need to be kept ultra-sterile inside the detector when they do the final installation. The team will need to be extra careful not to contaminate the area.

A speck of dust inside can create enough background noise in the form of subatomic particles that drown out a WIMP signal. The crew will have to wear white coveralls and booties to prevent contamination. Even a dropped tool risks embedding impurities in the floor.

There is another big challenge, as well. When they finally install the sensors, the titanium container and the acrylic tanks will already be set up inside the stainless steel vat. This will leave only a three-foot wide area around the detector’s inside perimeter for them to work in. They will build the scaffolding for the sensors one piece at a time, moving around the perimeter. Finally, they will end at the small entrance and exit portal.

Penning and his crew will bring a ladder with them to erect the scaffolding. But when the scaffolding is completed, there won’t be enough room to maneuver the ladder. The ladder is 10 feet; the exit is a 4-foot wide portal. The only solution is a custom-made ladder that can be taken apart or folded into the size of a suitcase.

Penning likens the entire construction process to “building a ship in a bottle,” though in this instance they will be working from within the bottle.

If everything goes as planned, the whole contraption will become operational in 2020 and run for three years. Penning is guardedly optimistic. “Our experiment is the one with the best chance in the next few years if nature is kind,” Penning says. “But what nature does isn’t up to us. We just discover it.”

Source: Brandeis University

  • Is the Higgs boson actually a ‘portal to the dark world’?
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    Tiny detector is 1st to see neutrinos bump nucleus

    (Credit: U. Chicago)

    In 1974, a physicist predicted a new way for ghostly particles called neutrinos to interact with matter. More than four decades later, the world’s smallest neutrino detector has observed the elusive interaction for the first time.

    Neutrinos are a challenge to study because their interactions with matter are so rare. Particularly elusive has been what’s known as coherent elastic neutrino-nucleus scattering, which occurs when a neutrino bumps off the nucleus of an atom.

    Researchers detected the scattering process by using a detector that’s small and lightweight enough for a researcher to carry.

    “Why did it take 43 years to observe this interaction?” asks Juan Collar, a physics professor at the University of Chicago and senior member of the Kavli Institute for Cosmological Physics. “What takes place is very subtle.”

    At the time, Freedman didn’t see much of a chance for experimental confirmation, writing: “Our suggestion may be an act of hubris, because the inevitable constraints of interaction rate, resolution, and background pose grave experimental difficulties.”

    When a neutrino bumps into the nucleus of an atom, it creates a tiny, barely measurable recoil. Making a detector out of heavy elements such as iodine, cesium, or xenon dramatically increases the probability for this new mode of neutrino interaction, compared to other processes. But there’s a trade-off, since the tiny nuclear recoils that result become more difficult to detect as the nucleus grows heavier.

    “Imagine your neutrinos are ping-pong balls striking a bowling ball. They are going to impart only a tiny extra momentum to this bowling ball,” Collar says.

    To detect that bit of tiny recoil, researchers figured out that a cesium iodide crystal doped with sodium was the perfect material. The discovery led the scientists to jettison the heavy, gigantic detectors common in neutrino research for one similar in size to a toaster.

    The 4-inch-by-13-inch detector used to produce the results weighs only 32 pounds (14.5 kilograms). In comparison, the world’s most famous neutrino observatories are equipped with thousands of tons of detector material.

    “You don’t have to build a gigantic laboratory around it,” says doctoral student Bjorn Scholz, whose thesis will contain the result reported in Science.

    “We can now think about building other small detectors that can then be used, for example to monitor the neutrino flux in nuclear power plants. You just put a nice little detector on the outside, and you can measure it in situ.”

    Mysterious particles

    Neutrino physicists, meanwhile, are interested in using the technology to better understand the properties of the mysterious particle.

    “Neutrinos are one of the most mysterious particles,” Collar says. “We ignore many things about them. We know they have mass, but we don’t know exactly how much.”

    Physicist says data from neutrino experiment are ‘gorgeous’

    Through measuring coherent elastic neutrino-nucleus scattering, physicists hope to answer such questions. The new paper, for example, imposes limits on new types of neutrino-quark interactions that have been proposed.

    The results also have implications in the search for Weakly Interacting Massive Particles. WIMPs are candidate particles for dark matter, which is invisible material of unknown composition that accounts for 85 percent of the mass of the universe.

    “What we have observed with neutrinos is the same process expected to be at play in all the WIMP detectors we have been building,” Collar says.

    Neutrino alley

    The COHERENT Collaboration, which involves 90 scientists at 18 institutions, has been conducting its search for coherent neutrino scattering at the Spallation Neutron Source at Oak Ridge National Laboratory in Tennessee. The researchers installed their detectors in a basement corridor that became known as “neutrino alley.” This corridor is heavily shielded by iron and concrete from the highly radioactive neutron beam target area, only 20 meters (less than 25 yards) away.

    ‘Ice fishing’ for neutrinos yields new measurements

    This neutrino alley solved a major problem for neutrino detection: It screens out almost all neutrons generated by the Spallation Neutron Source, but neutrinos can still reach the detectors. This allows researchers to more clearly see neutrino interactions in their data. Elsewhere they would be easily drowned out by the more prominent neutron detections.

    The Spallation Neutron Source generates the most intense pulsed neutron beams in the world for scientific research and industrial development. In the process of generating neutrons, the SNS also produces neutrinos, though in smaller quantities.

    “You could use a more sophisticated type of neutrino detector, but not the right kind of neutrino source, and you wouldn’t see this process,” Collar says. “It was the marriage of ideal source and ideal detector that made the experiment work.”

    The National Science Foundation, Alfred P. Sloan Foundation, US Department of Energy, and the Kavli Institute for Cosmological Physics funded the work.

    Source: University of Chicago