High School Student Earns Accolades for Summer Research with Gorshkov Group

Jason Youm, a high school student who performed summer research with Alexey Gorshkov, an adjunct associate professor of physics at UMD, in 2023, placed in the top dozen competitors in the physics and astronomy category at the Regeneron International Science and Engineering Fair (ISEF). In the competition, Youm, who recently completed his junior year at Montgomery Blair High School in Silver Spring, Maryland, presented research he completed under the mentorship of Gorshkov and Joseph Iosue, a graduate student in physics at UMD.

The Regeneron ISEF brings together high school students from across the world who earn their spots by qualifying at local science fairs. In his project, Youm performed calculations to help researchers investigate how quantum computers can perform certain tasks significantly faster than their traditional counterparts.

“I'm truly, really thankful for the research opportunity,” Youm said. “I think it's honestly changed my life. It's truly an invaluable experience.”Jason YoumJason Youm

Youm had harbored an interest in quantum physics for the first couple of years of high school, and after finishing his first calculus class during his sophomore year, he decided to look for opportunities to explore the interest more deeply. 

“Kind of on a whim, in mid-May, I just emailed some professors at UMD, because I heard they had a good program in quantum physics,” Youm said. “I just asked like, ‘I'm interested in these fields. Would you be interested in having a student intern during the summer?’ And Alexey was kind enough to accept me into the group.”

Gorshkov first looked over the relevant experience in math and physics Youm shared in his email and then reached out to the other members of the group to ask if any of them had a suitable project.

One of those graduate students, Iosue, was particularly interested in mentoring someone since he knew firsthand how valuable such experiences can be. When he was an undergraduate at the Massachusetts Institute of Technology (MIT), he had spent a summer working in Gorshkov’s group.

“My time as an undergrad in Alexey’s group was a very good experience for me,” Iosue said. “It was the best research experience I had until I started my Ph.D. So, I wanted to do something similar for someone else.”

Iosue remembered a project from his early days as a graduate student that had a natural continuation. The group hadn’t followed up on the possibility yet, and he thought the remaining work might be a suitable project for a motivated high school student.

The project developed mathematical tools for studying quantum entanglement—a phenomenon where the evolving fates of quantum particles become inextricably linked. A collection of quantum states can have different amounts of quantum entanglement that are possible, and Iosue performed calculations that help quantify if the quantum entanglement values are tightly or loosely clumped together. Entanglement plays a central role in quantum computers, so it is likely to be a key ingredient in any proof that quantum computing’s advantage is real and that a cleverly designed program on a traditional computer can’t possibly compete. 

The calculations that Iosue had performed were only the first of a set that each provide slightly different insights about the entanglement of the analyzed states. Iosue suggested that Youm could perform the other calculations by using the previous work as a guide. Gorshkov agreed, and Youm ended up taking on the project.

“My hope was that the calculations would be similar—like the whole beginning to end process that we did would be similar,” Iosue said. “So, it seemed like a high school student wouldn't have to necessarily dive into too much scientific literature or dive into too much uncertainty. I was hoping there was a bit more of a straight path, but with research, it's not always what you expect.”

Early in the summer, the project hit a snag. Iosue suggested Youm begin with a scientific paper that provided equations that were the natural starting point for the new calculations. But as Youm worked, his results weren’t going anywhere. When the group dug deeper, they determined that the equations in the paper were incorrect, and they had to start over by deriving the initial equations themselves.

Eventually, Youm successfully worked through the math for an additional portion of the calculations, and he also used computer simulations to verify his results.

“In the middle of the project was a lot of coding, mathematical work, and trying to understand the physics processes behind all the math that I was doing,” Youm said. “I worked for around eight hours a day, just trying to progress in my work and deriving the necessary formulas and the theorems. So it was pretty intensive, but also I really enjoyed it.”

In Youm’s science fair project, titled “Measuring Quantum Entanglement Entropy in Gaussian Boson Sampling,” he presented the results and discussed their practical applications to quantum experiments. The calculations apply to Gaussian boson sampling experiments where several measurements collect a sample of results from a specific set of prepared quantum states. Quantum mechanics allows a sample to be designed so that it reflects very specific statistics, and many physicists believe that for many cases it can be prohibitively complex for any computer not exploiting quantum phenomena to create a sample with the correct statistics.

The calculations that Youm performed are not directly used in sampling experiments, but they are a potential tool for studying how entanglement relates to the complexity of the sampling task. Understanding entanglement could be central to definitively proving if a sampling experiment has truly achieved an unassailable quantum advantage.

After the summer, Youm continued to work with the group—scheduling meetings around his normal school schedule and assignments. During the school year, Youm took the lead on writing a paper about the results, which the group has posted on the arXiv preprint server

“I've had high school students working with my group in the past, but this was the first time we worked over the summer with a rising junior instead of a rising senior,” said Gorshkov. “Jason's performance was outstanding!”

This summer Youm is once again took on a research project, but this year he was at the 2024 Center for Excellence in Education Research Science Institute summer program at MIT, which accepts 100 high school students from around the world. 

“I am really thankful for Alexey, and the rest of the research group, because without them I wouldn't have been able to get any of these opportunities,” Youm said. “I owe all of this to them, and I just feel really happy and grateful.”

Written by Bailey Bedford

 

In addition to Gorshkov and Iosue, QuICS Hartree Postdoctoral Fellow Yuxin Wang and JQI graduate student Adam Ehrenberg also worked with Youm and are authors on the paper posted on the arXiv preprint server.

Solving the Mystery of the Stinky Vapor Plumes on Campus

Billowing white columns of vapor rise silently from sidewalks and manholes around the University of Maryland campus when it gets chilly. These mysterious plumes are sometimes accompanied by a strange odor or a lingering warmth. Like ghosts, the hazy wisps seem to come and go without much explanation. But what’s the cause of this foggy, strange smelling campuswide phenomenon and where is it coming from? 

“It’s definitely not intentional or desirable,” said UMD Physics Professor Daniel Lathrop. “You’re not supposed to see or smell it at all. In fact, it’s just one component of a much bigger problem. This visible vapor is a sign that our underground utilities infrastructure is aging and inadvertently helping to cause water and heat waste across our campus.”Dan Lathrop. Credit: Georgia JiangDan Lathrop. Credit: Georgia Jiang

Like a leaky pipe, this leaking vapor can cause serious problems including infrastructure damage, energy waste and pollution to the natural areas surrounding UMD. 

The university’s infrastructure—some of which dates back over 150 years—naturally deteriorated over time. That includes the decades-old tri-generation energy system that the majority of the campus runs on today.

“Our current energy generation system was installed in 1999. It heats, cools and powers over 250 campus buildings,” explained Lathrop, who also holds joint appointments in the Departments of Geology and Physics, the Institute for Physical Science and Technology, and the Institute for Research in Electronics and Applied Physics. “A natural gas-fired turbine generates most of the electricity we use and the heat that this turbine produces is recaptured to produce steam, which produces additional electric power. The steam is then also used to heat and cool our buildings.” 

Gregg Garbesi, assistant director of utilities and energy management at UMD’s Facilities Management, says the visible vapor comes when liquid (like groundwater, city water leaks, stormwater leaks, etc.) physically contacts the underground steam line. He compares the campus’ visible vapor to steam caused by pouring cold water into a hot pan on a stove. He explains that the odd smells accompanying the vapor occur when organic materials come into contact with the leaked vapor, which is generated underground or in a steam manhole. 

According to Garbesi, seeing these vapor plumes signals energy loss. 

“For every pound of vapor generated, a pound of steam is condensed in the steam pipes,” he said. “All the energy that went into making that pound of steam—which could have been used to power campus—is lost, and if 100% of the condensate doesn’t return to the energy plant, that water is also lost.”

“We’re wasting about a million gallons of water a day now,” Lathrop added. “The loss in 2019 alone is estimated to be 700 million gallons, costing us an estimated $4 to $6 million a year. And that’s just the financial price tag that we know about.”

That’s why Lathrop is leading a multidepartment, cross-disciplinary Grand Challenges team that aims to map and pinpoint locations where steam is being lost and get a better look at challenges with energy consumption, water quality, methane emissions and air quality on UMD’s campus. With colleagues and students from the Departments of Geology, Atmospheric and Oceanic Science, Geographical Sciences, and Environmental Science and Technology, Lathrop hopes to tackle these interrelated issues by pinpointing the biggest problems and providing concrete solutions.

“Methane emissions, carbon dioxide emissions and pipeline water loss from our campus play a big role in stream water and air contamination nearby,” he said. “It’s our goal to measure these impacts and figure out how we can remediate these challenges to reduce our campus’ climate footprint and improve the environment here.”

Diagnosing and treating an aging energy system

When Lathrop began this project in spring 2023, his first step was to work with Facilities Management to learn more about the campus’ utilities-related challenges, particularly the steam issues caused by underground pipelines. He soon realized that his ongoing U.S. National Science Foundation-funded research—to develop sensors capable of detecting geophysical anomalies—could play a key part in this new project. 

“My lab was originally developing geophysical sensors to look for landmines and unexploded ordnance, but we recognized that this same system could be used to find buried utilities,” Lathrop explained, referring to a project that was named a UMD Invention of the Year in May 2022

Licensed drone pilot and physics senior Meyer Taffel is test-flying a drone over campus to magnetically map UMD's underground utilities. Credit: Dan LathropLicensed drone pilot and physics senior Meyer Taffel is test-flying a drone over campus to magnetically map UMD's underground utilities. Credit: Dan LathropUsing these sensors and historic infrastructure blueprints provided by Facilities Management, Lathrop and his team sketched out an extensive map of steam-emitting sources on campus. They concluded that UMD’s energy system had at least 55 active steam vents. 

A group of undergraduate physics majors taking Lathrop’s PHYS 499X class added to those findings when they hand-built a calorimeter (an instrument that measures heat from chemical and physical reactions) in fall 2023 as a course project. 

The students used the calorimeter to identify dozens of campus hot spots and learned that some of these accidental vents lost more than 60 kilowatts of heat energy via escaped condensation. For reference, a standard incandescent light bulb uses about 60 watts of electricity on average—meaning that the steam and heat leaking from some of these vents could power approximately 1,000 of those light bulbs. 

Lathrop estimates that this loss alone could equate to approximately $50,000 per year but he believes that identifying and analyzing the factors that led to the hot spots was invaluable.

“This is a team effort and having everyone on the same page can really make a difference when it comes to fixing things on campus and allocating resources appropriately. Our work has already started to help the university identify and patch sites on campus with water leaks,” he said. “We were able to prevent local building damage and protect students, staff and faculty from potential safety hazards.”

Putting together pieces of a bigger puzzle

Other members of the Grand Challenges project team are also on the ground looking for ways to locate and address the campus’ interconnected water and air quality problems.

Geology graduate student Julia Famiglietti and Geology Chair and Professor James Farquhar tracked gas leaks on campus through the sewer system to create a methane inventory (list of methane sources and sinks). They identified a contamination source underground that they suspect is related to the aging steam system.

“We think that the contamination has something to do with steam additives accidentally coming into contact with and reacting to methane,” explained Famiglietti, who sampled the air in campus sewers at least once a month to determine the composition of gases found in emissions. “We’re focusing on understanding the chemistry behind this contamination signature and directly discussing with the steam plant management personnel how to address the problem.” 

Geology Associate Professor Karen Prestegaard and Professor Sujay Kaushal found similar results while working with student groups to monitor the water quality of streams and storm drains. They discovered that water discharging from steam vents into storm drains had noticeably higher pH values and higher salt contamination than natural rainwater—potentially encrusting pipes with buildup and impacting wildlife in the Paint Branch waterways. 

Other efforts to gather and analyze the researchers’ environmental data include Project Greenhouse, in which First-Year Innovation & Research Experience (FIRE) undergraduates are drafting a sustainable methane budget for UMD.

Lathrop hopes that this multiyear campuswide team effort will help UMD reduce water and steam waste (and the associated environmental and fiscal costs) by 30% by the end of the project in June 2026. He believes this project can serve as a model for other research efforts to analyze similar urban environmental impacts for cities or large organizations like universities. 

“Our campus is a microcosm of urban and suburban environmental impacts, so evaluating UMD’s impact on the environment leads to a better understanding of how humans impact climate on a local, national and global level,” Lathrop said. “We’re all doing our part to protect our campus and the people living and working here.” 

Written by Georgia Jiang

 Other UMD faculty members involved in the Remediation of Methane, Water, and Heat Waste Grand Challenges project include Atmospheric and Oceanic Science Professor Russell Dickerson, Environmental Science and Technology Associate Professor Stephanie Yarwood, FIRE Assistant Clinical Professor Danielle Niu, Geographical Sciences Assistant Professor Yiqun Xie, and Geology Professors Michael Evans and Vedran Lekic. 

UMD Physicists Advance NASA’s Mission to ‘Touch the Sun’

Those who say there’s “nothing new under the sun” must not know about NASA’s Parker Solar Probe mission. Since its launch in 2018, this spacecraft has been shedding new light on Earth’s sun—and University of Maryland physicists are behind many of its discoveries.

At its core, the Parker Solar Probe is “on a mission to touch the sun,” in NASA’s words. It endures extreme conditions while dipping in and out of the corona—the outermost layer of the sun’s atmosphere—to collect data on magnetic fields, plasma and energetic particles. The corona is at least 100 times hotter than the sun’s surface, but it’s no match for the spacecraft’s incredible speed and carbon composite shield, which can survive 2,500 degrees Fahrenheit. Last year, the spacecraft broke its own record for the fastest object ever made by humans.

This engineering feat was built to solve solar mysteries that have long confounded scientists: What makes the sun’s corona so much hotter than its surface, and what powers the sun’s supersonic wind? These questions aren’t just of interest to scientists, either. The solar wind, which carries plasma and part of the sun’s magnetic field, can cause geomagnetic storms capable of knocking out power grids on Earth or endangering astronauts in space.

To better understand these mechanisms, the Parker Solar Probe will attempt its deepest dive into the corona on December 24, 2024, with plans to come within 3.9 million miles of the sun’s surface. Researchers hope its findings will help them predict space weather with greater accuracy and frequency in the future.

James Drake, a Distinguished University Professor in UMD’s Department of Physics and Institute for Physical Science and Technology (IPST), is helping to move the needle closer to that goal as a member of the Parker Solar Probe research team.

“This mission is what's called a discovery mission, and with a discovery mission we can never be sure what we're going to find,” Drake said. “But of course, everybody is most excited about the data that will come from the Parker Solar Probe getting very close to the sun because that will reveal new information about the solar wind.” 

Reconnecting the dots

Drake and Marc Swisdak, a research scientist in UMD’s Institute for Research in Electronics & Applied Physics (IREAP), have been involved with this mission since its inception. The researchers were asked to join because of their expertise in magnetic reconnection, a process that occurs when magnetic fields pointing in opposite directions cross-connect, releasing large amounts of magnetic energy.

Before the Parker Solar Probe, it was known that magnetic reconnection could produce solar flares and coronal mass ejections that launch magnetic energy and plasma out into space. However, this mission revealed just how important magnetic reconnection is to so many other solar processes. 

Early Parker Solar Probe data showed that magnetic reconnection was happening frequently near the equatorial plane of the heliosphere, the giant magnetic bubble that surrounds the sun and all of the planets. More specifically, this activity was observed in the heliospheric current sheet, which divides sectors of the magnetic field that point toward and away from the sun. 

“That was a big surprise,” Drake said of their findings. “Every time the spacecraft crossed the heliospheric current sheet, we saw evidence for reconnection and the associated heating and energization of the ambient plasma.”

In 2021, the Parker Solar Probe made another unexpected discovery: the existence of switchbacks in the solar wind, which Drake described as “kinks in the magnetic field.” Characterized by sharp changes in the magnetic field’s direction, these switchbacks loosely trace the shape of the letter S.

“No one predicted the switchbacks—at least not the magnitude and number of them—when Parker launched,” Swisdak said. 

To explain this odd phenomenon, Drake, Swisdak and other collaborators theorized that switchbacks were produced by magnetic reconnection in the corona. While the exact origin of those switchbacks hasn’t been definitively solved, it prompted UMD’s team to take a closer look at magnetic reconnection, especially its role in driving the solar wind.

“The role of reconnection has gone from something that was not necessarily that significant at the beginning to a major component of the entire Parker Solar Probe mission,” Drake said. “Because of our group's expertise on the magnetic reconnection topic, we have played a central role in much of this work.”

Last year, Drake and Swisdak co-authored a study with other members of the Parker science team that explained how the sun’s fast wind—one of two types of solar wind—can surpass 1 million miles per hour. They once again saw that magnetic reconnection was responsible, specifically the kind that occurs between open and closed magnetic fields, known as interchange reconnection.

To test their theories about solar activity, the UMD team also uses computer simulations to try to reproduce Parker observations. 

“I think that one of the things that convinced people that magnetic reconnection was a major driver of the solar wind is that our computer simulations were able to produce the energetic particles that they saw in the Parker Solar Probe data,” Drake said. 

As part of his dissertation, physics Ph.D. student Zhiyu Yin built the simulation model that is used to see how particles might accelerate during magnetic reconnection.

“Magnetic reconnection is very important, and our simulation model can help us connect theory with observations,” Yin said. “I'm really honored to be part of the Parker Solar Probe mission and to contribute to its work, and I believe it could lead to even more discoveries about the physics of the sun, giving us the confidence to take on more projects in exploring the solar system and other astrophysical realms.”

Swisdak explained that simulations also help researchers push past the limitations of space probes.

“Observations are measuring something that is real, but they’re limited. Parker can only be in one place at one time, it has a limited lifetime and it’s also very hard to run reproducible experiments on it,” Swisdak said. “Computations have complementary advantages in that you can set up a simulation based on what Parker is observing, but then you can tweak the parameters to see the bigger picture of what we think is happening.”

‘Things no one has seen’

There are still unsolved mysteries, including the exact mechanisms that produce switchbacks and drive the solar wind, but researchers hope that the Parker Solar Probe will continue to answer these and other important questions. The sun is currently experiencing more intense solar flares and coronal mass ejections than usual, which could yield new and interesting data on the mechanisms that energize particles in these explosive events.

This research also has wider relevance. Studying the solar wind can help scientists understand other winds throughout the universe, including the powerful winds produced by black holes and rapidly rotating stars called pulsars. Winds can even offer clues about the habitability of planets because of their ability to deflect harmful cosmic rays, which are forms of radiation.

“One of the reasons why the solar wind is important is because it protects planetary bodies from these very energetic particles that are bouncing around the galaxy,” Drake said. “If we didn't have that solar wind protecting us, it's not totally clear whether the Earth would have been a habitable environment.”

As the spacecraft prepares for its December descent into the sun, the UMD team is eager to see what the new observations will reveal.

“One of the nice things about being involved with this mission is that it’s a chance to make observations of things that no one has seen before. It lets you go into a new regime of space and say, ‘Alright, we thought things would look this way, and inevitably they don't,’” Swisdak said. “The ability to get close enough to the sun to see where the solar wind starts and where coronal mass ejections begin—and being able to take direct measurements of those phenomena—is really exciting.”

The Many Wonders of Uranium Ditelluride

In the menagerie of exotic materials, superconductors boast their own vibrant ecosystem.

All superconductors allow electricity to flow without any resistance. It’s their hallmark feature. But in many cases, that’s where the similarities end.

Some superconductors, like aluminum, are conventional—run-of-the-mill, bread-and-butter materials that are well understood and hold no surprises. Others are deemed unconventional: They are not yet fully understood, but that seem to follow a known pattern. But one material—uranium ditelluride (UTe2)—defies classification, continuously baffling scientists with a plethora of unexpected behaviors. 

“At first, we thought this was going to be another interesting superconductor like some other uranium compounds that have been studied in the past,” says Johnpierre Paglione, a professor of physics at the University of Maryland (UMD) and the director of the Quantum Materials Center (QMC). “But at this point, it's gone beyond that. And it's become a much richer example of how crazy a superconductor can get.”

Most superconductors start doing their resistance-less thing when they get super cold. But temperature is only one of the knobs available to researchers studying a material in the lab. Some materials slip into superconductivity when you dial in other aspects of their environment, like the pressure they’re subjected to or the strength of a magnetic field they’re bathed in. UTe2 isn’t fussy about these properties, and it happily hosts superconductivity in all kinds of different situations. And as researchers continue studying the material, they are finding more questions than answers. 

“This one material seems to do 100 different things,” says Nicholas Butch, who is a physicist at the National Institute of Standards and Technology (NIST) and a member of QMC. “Somebody asked me after one of my talks ‘What right does one material have to do all these things?’ and I said ‘Right?’”

Butch and Paglione, together with colleagues at UMD, NIST, QMC and elsewhere, have been at the forefront of exploring the many wonders of UTe2. Postdocs Shang Ran and Corey Frank, working at both NIST and QMC have spearheaded many of the efforts, from discovering superconductivity in the material to testing samples at National High Magnetic Field Laboratory facilities around the country and experimenting with different preparation techniques. And the buzz around UTe2 is catching on: QMC has been sharing the samples they synthesize with researchers at other universities, including the University of Illinois at Urbana-Champaign and Cornell University, and further study by these groups resulted in the discovery of yet more unexpected behaviors. Uranium ditelluride (UTe2)Uranium ditelluride (UTe2)

A serendipitous discovery

Back in 2018, UMD and NIST postdoc Shang Ran was trying to synthesize U7Te12—a mixture of uranium and tellurium that’s predicted to have intriguing magnetic properties. Instead, Ran kept accidentally making UTe2. He found some literature from the 1960s suggesting UTe2 might have some interesting magnetic properties as well, and after consulting Butch, the two decided to cool it down anyway to see what would happen. Ran stuck the sample into a special helium-powered refrigerator. To his surprise, superconducting currents started to flow.

“We accidentally synthesized this uranium ditelluride, and it turned out it’s a superconductor. So, miracle!” Ran says. “That certainly brought excitement to the community and to our research.”

Ran became captivated with UTe2, and the team went on to poke and prod at it to try to understand its superconducting properties. To start, they set out to explore one of the key behaviors for any superconductor—its response to a magnetic field.  

In superconductors, electrons floating around in the material couple up, forming what’s known as Cooper pairs. These pairs act in concert with each other, and with the other pairs around them, allowing the electrons to flow without resistance. However, a strong magnetic field can break up the pairs, destroying the superconducting magic. One of the main signatures of a superconductor is how much magnetic juice it can withstand, and Ran and his collaborators set out to find this landmark for uranium ditelluride. 

To their surprise, uranium ditelluride remained a superconductor as they turned the field all the way up to the maximum power they has access to in the lab—20 tesla. That’s the combined magnetic strength of about two thousand fridge magnets, or ten times the magnetic field in an MRI machine. “I was shocked when [graduate student Chris Eckgerg] showed me the data,” says Ran. “I asked him ‘Did you measure correctly?’ We measured again and it was all correct. So, we realized, okay, there's some very strange thing going on.”

It wasn’t until they brought the material to the National High Magnetic Field Laboratory in Tallahassee, Florida that they finally found a magnet strong enough to tear apart UTe2’s Cooper pairs: It took an astounding 35 tesla to break the bond. For comparison, the first superconductor ever discovered—mercury—loses its superconductivity at a mere 0.1 tesla. This tipped off Ran, Butch, and the others that UTe2 was no conventional superconductor. They guessed that the electrons inside UTe2 form Cooper pairs in an unusually resilient way.

A special kind of dance

The electrons in a superconductor are kind of like a group of couples on a dance floor. In conventional superconductors, the electron pairs dance together in a straight line, a simple dance where partners mirror each other known as spin-singlet pairing. This synchronized movement allows them to glide effortlessly across the dance floor without any hindrance. However, in some unconventional superconductors, the electron pairs dance in swirly circles, spinning around each other as they glide across the dance floor. This unique dance style, known as spin-triplet pairing, gives them a different kind of coordination.

One consequence of this swirly dance pattern is that breaking up the partners with a magnetic field is much harder, which would explain the high magnetic field UTe2 could withstand. To check if that was going on inside UTe2, the QMC team collaborated with the group of Yuji Furukawa at Iowa State University. The Iowa team used their best techniques for distinguishing between the electron dance patterns, nuclear magnetic resonance spectroscopy. These studies confirmed Ran’s suspicions that UTe2 is a rare spin-triplet superconductor

Fewer than a dozen materials are suspected of spin-triplet pairing, and the other candidates are difficult to study—they are either hard to synthesize reliably or they only become superconducting under intense pressures or extremely low temperatures. Uranium ditelluride appears to be the most user-friendly spin-triplet superconductor to date, presenting a rare opportunity for researchers. 

“This is the only triplet superconductor I know that can be studied by so many different probes,” says Vidya Madhavan, a condensed matter physicist and professor at the University of Illinois at Urbana-Champaign (UIUC) who is a longtime collaborator of the QMC team. 

In addition to satisfying a physicist’s basic curiosity, spin-triplet superconductors might be useful as platforms for quantum computing. Spin-triplet pairing is a necessary ingredient for a yet rarer property that hasn’t been confirmed in any superconductor to date—a non-trivial topology. If spin-triplet pairing imbues electron couples with killer dance moves, a non-trivial topology warps the whole dance floor with curves and twists, radically changing the dance patterns of all the couples en masse. 

In the months following the discovery of UTe2’s swirly dance patterns, some evidence suggested that UTe2 might not only be a spin-triplet superconductor but also possess that topological special sauce. The evidence is not yet conclusive, but researchers are hard at work trying to sort this out, as well as understand more about what makes UTe2 tick. And their sleuthing keeps turning up more surprises. 

Superconductivity raised from the dead (and the never-born)

Ran and his labmates were wondering why 35 tesla seemed to be the magic number that broke superconductivity in UTe2. In search of clues, they went back to the National High Magnetic Field Lab.  They kept turning up the magnetic field even higher, looking at how the non-superconducting chunk responded. They also tilted the sample, putting the magnetic field off-kilter from UTe2’s natural crystal structure. 

Shockingly, as they kept rotating the sample, superconductivity reappeared at a field of 40 tesla. This was strange. Turning the field up really high killed the superconductivity, but if you kept going it came back to life. This phenomenon was termed Lazarus superconductivity after the biblical figure raised from the dead. Lazarus superconductivity is extremely rare, though not entirely unprecedented. It’s cropped up in a handful of materials before, and scientists think they have plausible mechanisms for explaining the effect. But none of those mechanisms seemed applicable to UTe2. 

In 2020, Ran joined the physics department at Washington University in St Louis, passing the torch of Butch’s QMC lab to a new postdoctoral researcher, Corey Frank. Frank had just completed her PhD in solid-state chemistry—the perfect background for mastering different ways of concocting the UTe2 crystal. She played with the initial concentrations of the starting materials as well as precise techniques and temperatures of preparation. Among other things, Frank developed a protocol for making UTe2 samples that are just shy of superconducting by making them intentionally just a bit dirty, peppering the crystals with purposefully introduced defects. These defects gum up the pathways by which electrons pair up and find their dance partners, preventing the development of superconductivity. “You can learn a lot about a phase by studying what kills it,” Frank says. 

Frank and her colleagues made a purposefully dirty sample and took it with them on another trip to the National High Magnetic Field Laboratory, this time in Los Alamos, New Mexico. They stuck the sample into the huge magnets and cranked up the field. Once the field was high enough and the sample had the right orientation, the resistance through the material dropped to zero—superconductivity was revived. 

“I was so excited,” Frank recalls. “You're not allowed to jump when you're on the platform of a high-field magnet, but I had to get down from the magnet so I could jump. It was amazing.”

This was completely unprecedented. In all the previous Lazarus superconducting materials, the mechanism behind the rebirth was presumed to involve recreating the conditions at a low magnetic field. Here, recreating conditions at a low magnetic field would not result in superconductivity because the samples had intentional defects, and yet there it was—superconductivity raised not from the dead, but from the never-born, a high-field superconducting phase all its own. The team reported this phenomenon last year in a preprint.

“We know how high field superconductivity works, the rules that govern that, and this one breaks those rules,” Frank says. “So the fact that we have this much more robust high-field phase is wild. I cannot overemphasize how unexpected it is.” 

The authors have some ideas of what could be causing this behavior, and they say further experiments are needed to figure out if those ideas are correct. For now, the experiments are on hold as they require even stronger magnetic fields than the National High Magnetic Field Laboratory currently offers. In the meantime, the QMC team is still studying how this superconductivity dies, comparing their revived samples to others in search of a pattern. 

Making waves 

Over many years Ran, Frank, and other members of the Butch lab have mastered the dual feats of growing pure uranium ditelluride crystals and studying their overall behavior—superconductivity, response to magnetic fields, and more. But they lacked the tools and expertise to zoom in on the microscopic, atom-by-atom behavior of UTe2. So they’ve enlisted the help of Vidya Madhavan’s team at UIUC.

In her lab, Madhavan has a scanning tunneling microscope (STM). An STM works by bringing a bit of metal tapered down to a tiny, fine point extremely close to the surface of a sample—so close that electrons from the sample can hop over to the conducting tip, or vice versa. By measuring how many electrons make the jump, scientists can learn a lot about the microscopic structure of a material, including where the electrons are on the surface of the sample.

The Butch group sent Madhavan a sample, and Anuva Aishwarya, a graduate student at UIUC who led the study, placed a sample of UTe2 into the scanning tunneling microscope. The team cooled the material just shy of its superconducting temperature, and they stumbled upon another surprise: The electrons didn’t follow the ups and downs of UTe2’s crystal structure. Instead, they clustered together and then apart, forming waves of charge frozen into the surface with a pattern all their own.

These kinds of charge density waves are uncommon but not unprecedented. However, the measurements performed by Ran, Frank or others at QMC didn’t show any indication that a charge density wave might be found in UTe2. To Madhavan and her team, this came out of nowhere.

To try to understand what they were seeing, Aishwarya and her lab mates probed the behavior of these waves in different temperatures and magnetic fields. They found that, in a magnetic field, the charge density wave seemed intimately related to superconductivity itself. As they turned up the field, the charge density wave broke down at precisely the same field strength as superconductivity. This tipped off Madhavan and her collaborators at UIUC that maybe this wave had some relationship to the superconductivity in uranium ditelluride.

If you want to pick out individual electrons, a regular STM is great. But if you want to peer inside the dance patterns of electron couples in a superconductor, you need an STM armed with a special kind of tip—one that is itself a superconductor. The team of Seamus Davis at Cornell University had just such a superconducting tip. They became intrigued by Madhavan’s results and got in on the action. They obtained another sample from the QMC team and stuck it in their specialized STM. They found that the electron pairs behaved similarly to the lone electrons. Here, too, the pairs clustered together and apart, forming a so-called pair density wave with the same beat as the charge density wave observed by Madhavan. This is the first time such a pair density wave has been found in a spin-triplet superconductor.

As with many aspects of UTe2, the origins of the charge and pair density waves remain far from clear. But, Ran comments, these waves are a fairly common feature in unconventional spin-singlet superconductors. This may provide clues for how all these different strange superconductors are connected. “We eventually need to understand unconventional superconductivity overall,” Ran says. “And having this common theme I think is very important for theorists.”

While theorists are hard at work trying to crack the puzzle of unconventional superconductivity, Ran, Butch, and other researchers are continuing to explore all that UTe2 has in store. “It's really rich. It’s a great place to explore,” says Butch. “This one material underscores how little we know about spin triplet physics. It’s as if we are writing textbooks about it right now. So that's actually very exciting.”

Story by Dina Genkina