UMD CMNS Physics S1 Color

As dark matter eludes scientists, they plan a more extensive search

carter imageThis empty honeycomb array in the LUX experiment now holds photomultiplier tubes, which are ready to catch light signals caused by dark matter. Photo by Carlos Faham.

For decades, scientists have suspected that the universe contains more matter than we can see.  They point to clues in the cosmos, such as irregularities in the radiation left over from the early universe and the way light bends around galaxies. By studying the rotation rates of galaxies, pioneering astrophysicists like the late Vera Rubin determined that about 85% of the mass in the universe doesn't betray its presence by emitting any light. For this reason, they named this mysterious mass dark matter.

Researchers from the University of Maryland (UMD), led by Associate Professor Carter Hall, have been blazing the trail in the search for dark matter. Their involvement with the Large Underground Xenon (LUX) experiment—the most sensitive detector of its kind—has placed the most stringent limits yet on the properties of dark matter. And now that LUX has finished taking data, the focus is shifting to the next generation of experiments. An even more sensitive detector called the LUX-ZEPLIN (LZ) experiment is already under construction, and Hall will soon begin a term as the spokesperson for the collaboration.

Since 2013, the LUX collaboration, which includes scientists from the United Kingdom, Portugal and across the United States, has been looking for dark matter in the form of weakly interacting massive particles, or WIMPs. WIMPs are a leading candidate for this mysterious matter, and LUX has been hunting them from an old gold mine in the Black Hills of South Dakota, nearly a mile underground.

The experiment, which consists of a tank with 375 kilograms of ultra-pure liquid xenon and a layer of xenon gas, tries to spot the telltale signs of a WIMP knocking into ordinary matter. Theory predicts that when a WIMP collides with a xenon nucleus, the nucleus will recoil and collide with other nearby xenon atoms. This sets off a chain reaction, liberating electrons from the atoms and releasing ultraviolet light in the process.

LUX sits and waits for this light. Photomultiplier tubes, which act like simple cameras, line the top and bottom of the tank, eyes peeled for quick flashes. An electric field corrals the free electrons toward the top of the tank, and they produce more light when they leap into the layer of xenon gas. These signals tell the researchers where in the detector the WIMP collision occurred. The researchers chose to use xenon in the LUX and LZ experiments because the xenon nucleus is very likely to interact with WIMPs. "It's also not too expensive," says Hall. "You can buy many tons of it."

The experiment must reject false signals, which requires exquisite control. For example, the team worked hard to shield the experiment from cosmic rays—the steady stream of particles from outer space that pass through your body 30 times every second. The mile of bedrock above the mine shields the experiment from these particles, as does a 6-meter- high tank of ultra-pure water surrounding the xenon. They also take care to use detector materials that don't spit out WIMP impostors like neutrons through radioactive decay.  

Hall and his UMD collaborators played crucial roles in the LUX collaboration. They provided a source of tritium, a radioactive isotope of hydrogen, to help calibrate the detector. They also built a system to screen the detector material—liquid xenon— for impurities. Richard Knoche, one of Hall's graduate students, recently defended his Ph.D. thesis on how to analyze data from LUX given that its electric field is not uniform.  

Different dark matter theories predict different properties for WIMPs, and no one knows how massive WIMPs are or how likely they are to react with ordinary matter. But every dark matter detector scientists build is more sensitive than its predecessor, and progress means putting stricter and stricter limits on the possible masses and interactions strengths a WIMP could have.

After an initial experimental run in 2013, the LUX team has continued to update the experiment, making it four times more sensitive to most WIMP masses. The collaboration did not identify any nuclear recoils due to WIMPs in their 2016 data, which confirms the findings reported by other dark matter searches.

The lack of observed WIMP events makes the continuing work in dark matter detectors even more important, and the next-generation LZ experiment will be 100 times more sensitive than LUX. It will be so sensitive, in fact, that it should be able to detect the constant stream of tiny and nearly massless neutrinos streaming toward us from the sun. Hall says that detecting this neutrino wind will be compelling evidence that LZ is functioning properly.

If LZ sees the neutrino wind and still doesn't spot any WIMPs, it could mean that a new approach to detecting dark matter is needed. Scientists have proposed other theories of what dark matter is, including another particle called the axion, and they may shift toward exploring those theories more seriously if LZ exhausts the search for WIMPs. The lack of discoveries from the Large Hadron Collider that would support the WIMP hypothesis has also caused scientists to take a step back and re-examine their theories on dark matter.

But if researchers are getting close to finishing the search for WIMPs, then LZ will play an important role in taking that those last steps. "There's another, at least, ten years of WIMP experiments that are now planned to be carried out," Hall says. The LZ detector, which is scheduled to start taking data in 2020, may provide the final word on many lingering questions surrounding dark matter.

More information about the LUX and LZ experiments can be found at and, respectively.

Written by Erin Marshall, UMD Physics

Research article reference:

"Results from a Search for Dark Matter in the Complete LUX Exposure," D. S. Akerib et al. (LUX Collaboration)
Phys. Rev. Lett. 118, 021303, (2017); APS Physics Viewpoint:

Selected popular news accounts on this research:



Paik's Work Cited as 2016 Highlight

Research Professor and Professor Emeritus Ho Jung Paik is the lead author of the article "Low-frequency terrestrial tensor gravitational-wave detector," which has been selected by the journal Classical and Quantum Gravity as one of their highlights of 2016. Postdoctoral associate Cornelius Griggs and research scientist Martin Vol Moody collaborated on the article. It presents a design concept for a tensor gravitational wave detector, capable of detecting certain interactions among white dwarf stars, neutron stars, and black holes in the new mid-frequency band of 0.1 to 10 Hz, at sensitivities much higher than other existing technologies. The proposed instrument, which utilizes six five-ton test masses and three orthogonal axes 30 m or longer, is based on the Tensor Superconducting Gravity Gradiometer being developed by the PICASSO program, which utilizes six 100-gram superconducting test masses with a 14 cm baseline.

Read more 


Probe for nanofibers has atom-scale sensitivity

Optical fibers are the backbone of modern communications, shuttling information from A to B through thin glass filaments as pulses of light. They are used extensively in telecommunications, allowing information to travel at near the speed of light virtually without loss.

Physics - Synopsis: Chemical Echo

Echoes are not limited to sound reflecting off cave walls. A similar phenomenon—a delayed response following an immediate response to some stimulus—can occur after coupled oscillators are stimulated by a sequence of two input pulses. Researchers have now observed such an echo phenomenon in a system of coupled chemical oscillators.  

Edward Ott of the University of Maryland in College Park, Kenneth Showalter of West Virginia University in Morgantown, and their colleagues studied a standard oscillating chemical system known as the Belousov-Zhabotinsky reaction. This light sensitive reaction involves transitions between an opaque state and one that transmits light. The team fixed more than 1000 tiny beads containing the relevant chemicals in a setup that allowed the beads—each with its own oscillation frequency—to be individually illuminated and the light transmitted through each bead to be separately detected.

A Warm Welcome for Weyl Physics

Warm welcome for weyl physics

This is part one of a two-part series on Weyl semimetals and Weyl fermions, newly discovered materials and particles that have drawn great interest from researchers at JQI and the Condensed Matter Theory Center at the University of Maryland. The first part focuses on the history and basic physics of these materials. Part two will focus on theoretical work at Maryland and will appear next week.

For decades, particle accelerators have grabbed headlines while smashing matter together at faster and faster speeds. But in recent years, alongside the progress in high-energy experiments, another realm of physics has been taking its own exciting strides forward.

That realm, which researchers call condensed matter physics, studies chunks of matter moving decidedly slower than the protons in the LHC. In fact, the materials under study—typically solids or liquids—are usually sitting still. That doesn't make them boring, though. Their calm appearance can often hide exotic physics that arises from their microscopic activity.

"In condensed matter physics, the energy scales are much lower," says Pallab Goswami, a postdoctoral researcher at JQI and the Condensed Matter Theory Center (CMTC) at the University of Maryland. "We want to go to lower energies and find new phenomena, which is exactly the opposite of what is done in particle physics."

Historically, that's been a fruitful approach. The field has explained the physics of semiconductors—like the silicon that makes computer chips—and many superconductors, which generate the large magnetic fields required for clinical MRI machines.

Over the past decade, that success has continued. In 2004, researchers at the University of Manchester in the UK discovered a way to make single-atom-thick sheets of carbon by sticking Scotch tape onto graphite and peeling it off. It was a shockingly low-tech way to make graphene, a material with stellar electrical properties and incredible strength, and it led quickly to a Nobel Prize in physics in 2010.

A few years later, researchers discovered topological insulators, materials that trap their internal electrons but let charges on the surface flow freely. It's a behavior that requires sophisticated math to explain—math that earned three researchers a share of the 2016 Nobel Prize in physics for theoretical discoveries that ultimately explain the physics of these and other materials.

In 2012, experimentalists studying the junction between a superconductor and a spotted evidence for Majorana fermions, particles that behave like uncharged electrons. Originally studied in the context of high-energy physics, these exotic particles never showed up in accelerators, but scientists at JQI predicted that they might make an appearance at much lower energies.

Last year, separate research groups at Princeton University, MIT and the Chinese Academy of Sciences discovered yet another exotic material—a Weyl semimetal—and with it yet another particle: the Weyl fermion. It brought an end to a decades-long search that began in the 1930s and earned acclaim as a top-10 discovery of the year, according to Physics World.

Like graphene, Weyl semimetals have appealing electrical properties and may one day make their way into electronic devices. But, perhaps more intriguingly for theorists, they also share some of the rich physics of topological insulators and have provoked a flurry new research. Scientists working with JQI Fellow Sankar Das Sarma, the Director of CMTC, have published 18 papers on the subject since 2014.

Das Sarma says that the progress in understanding solid state materials over the past decade has been astonishing, especially the discovery of phenomena researchers once thought were confined to high-energy physics. "It shows how clever nature is, as concepts and laws developed in one area of physics show up in a completely disparate area in unanticipated ways," he says.

An article next week will explore some of the work on Weyl materials at JQI and CMTC. This week's story will focus on the fundamental physics at play in these unusual materials.  

Take a closer look with part two of this series.