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News

Featured News

Image from E. coli research

UT’s Biophysics Research Lays the Groundwork for Designing New Antibiotics

December 17, 2024

Experiments with E. coli cells in microfluidic channels where their length response to FtsZ levels can be determined with 50 nm precision.

Bacteria may be microscopic in size, but anyone who’s suffered through strep throat or salmonella knows they can be tough opponents. Antibiotics keep bacterial cells from dividing, stopping them in their tracks and shutting down the infections they cause. But bacteria can mutate, outsmarting these medications and making them much less effective.

To come up with new therapies that prevent bacterial cells from dividing, scientists need to know the full story of how they divide. Professor Jaan Mannik and his colleagues have made an important step in that direction by identifying which proteins are rate-limiting for cell division. The results were published in Nature Communications.

Mannik’s group studies a common strain of Escherichia coli (E. coli), which provides a good baseline for the physics of how bacteria work. He described these cells as “little rods about one-thirtieth of the diameter of a hair” and anywhere from two to four micrometers in length. In ideal growth conditions, they can divide every 20 minutes.

“Division is one of the most fundamental cellular processes,” Mannik explained. “Several well-known antibiotics, including ampicillin and cephalexin, inhibit cell division. Bacteria whose division is inhibited die after a while. If we understand division better, new antibiotics can be designed.”

There’s a pressing need for new medicines because bacteria have gained an upper hand.

“Antibiotics have been losing their effectiveness because bacteria mutate rapidly, and antibiotics are used carelessly,” Mannik said. “The latter allows the mutations to take over in cell populations. Antibiotic-resistant bacteria are not a problem of the future but a current reality.”  

Certain elements of cell division in E. coli are understood. Scientists know it begins with the formation of a ring-shaped structure (the Z-ring) around the cell’s middle. The Z-ring organizes proteins to develop a septal wall. However, the formation of the Z-ring is not yet sufficient to trigger cells to constrict—a process responsible for splitting a mother cell into two daughters.

There are a few similar-sounding proteins at work here: FtsZ (Filamenting temperature-sensitive mutant Z), as well as FtsN and FtsA. Earlier research has shown that FtsZ is critical for forming the Z-ring, but Mannik and his colleagues were looking for its role in triggering the constriction, which happens long after the Z-ring has formed.

“We want to determine what mechanism triggers their division,” he said. “In other words, how (do) a bunch of proteins, such as FtsZ and FtsN, assemble in the cell and ‘decide’ that cell needs to divide?”

To discover what flips the switch, Jaan Mannik worked with Jaana Mannik, a research scientist in the department, as well as graduate student Chathuddasie Amarasinghe and colleagues from Harvard University and the Weizmann Institute of Science who modeled the division process. He said others in the field have thought FtsN was the key protein prompting cell division in E. coli, “but our research shows that it does not.”

The team got their experimental results using high throughput imaging in microfluidic devices—essentially a miniature lab on a quarter-size chip that lets researchers grow individual bacterial cells in microscopic channels, prod them with different stimuli, and then record their responses. Mannik said their key finding is that FtsZ accumulation controls when cells start to constrict. FtsZ numbers in the cell must reach a certain threshold level to trigger the process. This threshold level allows FtsZ filaments to form doublets or bundles, which recruit some other Fts-proteins and trigger a cascade of reactions needed for cells to constrict.

“If the constriction does not start to form, cells grow to long filaments and then die,” he said. “If we understand how this process takes place in E. coli and presumably also in other bacteria, then we can devise new means to stop it and thereby treat bacterial infections.”

December 17, 2024  |  Filed Under: Featured News, News, Soft Matter

A photo of Christine Nattrass

Research Takes UT Faculty and Students to the Extreme

December 12, 2024

Professor Christine Nattrass is among the College of Arts and Sciences faculty working in extreme environments. She talks about her nuclear physics research and the importance of moving the boundaries of what’s possible in this CAS feature.

December 12, 2024  |  Filed Under: Featured News, News, Nuclear

CMP theory research image

Understanding Cuprates of All Stripes

December 11, 2024

Steve Johnston doesn’t judge materials by their extended relatives. The department’s Bains Professor investigates how their physics can be different on a family-by-family basis as he studies what gives rise to superconductivity—electric current flowing with no resistance. Studies like these make crucial steps toward designing the quantum materials that will drive future technologies and economies.

In findings published in the Proceedings of the National Academy of Sciences (PNAS), Johnston and colleagues report how they used advanced computational modeling to show that not all families are alike and what those differences mean.

Single-Band Limits

Among the best-known high-temperature superconductors are cuprates—materials made from copper and oxygen. Discovered in 1986, they’ve been widely studied but still present a lot of unanswered questions. Theorists like Johnston have seen that the underlying properties—spin and charge and how those correlate—can be inconsistent across cuprate families. Sometimes the physics assists with superconductivity; sometimes it competes with it.

Johnston explained that in basic terms what happens in these materials is that copper and oxygen atoms form a plane. The standard for describing that system is the single-band Hubbard model.    

“You can think of it as removing oxygen from the plane to get this sort of effective copper-only description,” he said. “For years, people thought that really describes the physics.”

He said the model captures a lot of details that experiments have discovered about cuprates. It does a good job of showing how the electrons’ spins and charges form an alternating pattern of rows, or “stripes.” It accounts for the addition or subtraction of electrons from cuprate planes (called doping) that causes them to superconduct.

Yet there are limits to what this framework can do, especially in showing material-specific characteristics among different cuprate families.

“Everyone focused on these single-band descriptions because they’re easier to handle computationally,” Johnston said. “(If) you put the oxygen back in, it becomes a more complex problem and you need even more computational resources to solve it.”

Collaborating with partners from the University of Illinois and Oak Ridge National Laboratory (ORNL), Johnston and Research Assistant Professor Benjamin Cohen-Stead approached this complexity with the three-band Hubbard model, and used advanced algorithms and computing power to get a more detailed picture of the system.

Common Elements; Different Families

The single-band model predicts a reliable pattern for electronic charge and magnetism in cuprates. As Johnston explained, you can picture the “stripes” in cuprates as a kind of atomic board with alternating rows. One row will have lots of holes left by removing electrons while the next row will have no holes at all, and so on, in a repeating pattern. The phases of the charge in the hole-rich region and magnetism in the hole-depleted rows are locked with the neighboring regions.

“So, when the period of one changes, the period of the other changes,” he said. “That’s what’s seen experimentally in a lot of these systems and that’s what the single-band model predicts.”

The work he and fellow scientists reported in PNAS found something different.

Staggered spin (A) and charge (B) correlations at different hole densities in cuprates.

“What we’re finding in the three-band model is that (the stripes) are no longer coupled,” Johnston explained. “The spin and charge start to split apart; they’re no longer intertwined,” so you can independently change spin and charge modulations.

“If you take the single-model Hubbard model at face value, you basically expect all cuprates to be the same,” he said. “And we know that doesn’t happen experimentally. What this is telling you is that once you put the oxygen back in, you can start accounting for some of these differences that appear between bismuth-, lanthanum-, and yttrium-based cuprates. You can sort of understand these material-dependent factors. It’s an important step in separating out what’s universal and what’s material-specific.”

Knowing how different superconducting materials behave is the key to putting them to work.

“If we understand what makes a high-temperature superconductor superconduct, we have a better chance of engineering them,” Johnston explained. “In the end, we want to design materials and control the properties of these quantum systems with a high degree of precision.”

Efficient Teamwork

What makes this research possible is writing and running computational models to help scientists define a material’s properties. Johnston has long worked with colleague Thomas Maier of ORNL’s Computational Sciences and Engineering Division, who was a co-author on the PNAS paper. Maier is also a co-principal investigator on a National Science Foundation Elements grant Johnston won earlier this year. That award will help them expand a suite of codes called SmoQy that Johnston’s group developed.

Instead of coming up with a new model whenever a new material comes out, this library has codes ready to use from the get-go. (The SmoQy suite played a starring role in the PNAS research.) Johnston and Maier will build this collection further with another time saver. They’ll model a small part of an infinite system, then embed that model with an average approximation for the remainder of the system to account for all the quantum mechanics involved.

“We’re a computing university,” Johnston said of UT. “We’re very well-known for computing, so it makes sense that we develop these software stacks and help push the field forward using these tools.”

Technological progress like this includes the hard work of building a strong foundation. Two years ago, Johnston and Professor Hanno Weitering created a monolayer superconductor that landed on the cover of Nature Physics.

“That really grew out of our microscopic understanding of the Hubbard model and the physics of cuprate-like materials,” Johnston explained. “If you go back and look at the physics of semiconductors, the same thing happened there. Semiconductors were developed by people really trying to understand quantum theories of matter. That foundation has formed the basis for our entire modern economy. And it wouldn’t have happened without that fundamental research.”

December 11, 2024  |  Filed Under: Condensed Matter, Featured News, News

Artwork from Physics Magazine and ORNL

Spotting the Scars of Spacetime

December 6, 2024

From Physics Magazine:

“Scientists have devised a way to use current gravitational-wave detectors to observe permanent deformations of spacetime caused by certain supernovae.”

Graduate Student Colter Richardson is the lead author on the PRL that inspired this highlight. Fellow graduate student Michael Benjamin is among the co-authors, along with Professor Anthony Mezzacappa.

Read the full story.

This research was also featured as a National Science Foundation story and a highlight at phys.org and Physics World.

December 6, 2024  |  Filed Under: Featured News

Photo of fall 2024 Women in Physics lunch

Fall 2024 Women in Physics Lunch

December 5, 2024

Photo of fall 2024 women in physics lunch

The department held its fall 2024 Women in Physics Lunch on December 4, when more than 30 undergraduates, graduate students, post-docs, and faculty gathered to catch up while enjoying excellent food.

The president and vice-president of the Undergraduate Women in Physics group also introduced a Mentorship Matrix Program that will put together small groups of female undergrads, grads, post-doc and faculty to provide advice and mentorship. The program will start next semester. 

We thank the Department of Physics and Astronomy for the support provided, and we are looking forward to our next meeting, the 2025 edition on May 8, 2025. Save the date!

Courtesy of Professor Adriana Moreo

December 5, 2024  |  Filed Under: Featured News, News

Christmas Stargazing Event

Christmas Candlelight Tour and Stargazing

November 27, 2024

The Department of Physics and Astronomy is partnering once again with the Marble Springs State Historic Site for a night under the stars!

The December 13 event begins with storytelling as historic reenactors share tales of 18th-century holiday traditions. Next comes a tour through charming and festive candlelit cabins. Finally, our physics graduate students will share their knowledge of astronomy and guide visitors through the night sky with telescopes set up on the main lawn.

This event is perfect for families, history buffs, and anyone who loves a starry night under the open sky.

Admission is free and open to everyone! You can RSVP and learn more about the event in greater detail at: https://www.facebook.com/share/kB2uj3CGa8sNLk3y/

WHAT

Christmas Candlelight Tour and Stargazing

WHO

Everyone!

COST

Free

WHEN

Friday, December 13

Candlelight Tour | 5:30 PM – 7:00 PM

Stargazing with UT Physics & Astronomy | 7:00 PM – 11:00 PM

WHERE

Marble Springs State Historic Site

Need More Info? Call (865) 573-5508 or email the Marble Springs Program Coordinator at danielles@marblesprings.net.

Marble Springs State Historic Site is funded under an agreement with the Tennessee Department of Environment and Conservation Tennessee Historical Commission.

November 27, 2024  |  Filed Under: Featured News, News, Uncategorized

A photo of a student presenting research at the CPAD 2024 Workshop.

The (Particle) Detectorists

November 26, 2024

Photo of 2024 CPAD Workshop Attendees in front of Ayres Hall
2024 CPAD Conference Photo

If scientists want to know what makes up matter they have to sort and study the particles that compose it. That effort requires precision detectors. UT Physics and Oak Ridge National Laboratory (ORNL) hosted the 2024 Coordinating Panel for Advanced Detectors Workshop (CPAD) so physicists could exchange ideas about designing, building, and using these systems to explain how the universe works.

Some 260 participants attended the meeting, which ran November 19-22. With sessions covering topics from fast timing detectors to detector mechanics, they learned what works and what the next steps might look like in particle detection. They also had an opportunity to tour ORNL. Tova Holmes, an assistant professor of physics and a member of the workshop’s local organizing committee, explained why this research matters to everyone—not just scientists.

“Advancing detector technology drives our understanding of the universe,” she said, “but these detectors are also one of our most valuable contributions to society as particle physicists: modern medical scanning technology, nuclear non-proliferation technology; all of these emerge directly from particle physics. The CPAD workshop helps the community consolidate around the most promising ideas and drive them forward.”

In addition to the parallel and plenary sessions, students had the chance to share their research in a poster session, where UT’s Adam Vendrasco won a best poster design honorable mention for his project “Containerization of the Burn in Box Software for the CMS Outer Tracker Upgrade.” As a member of UT’s Compact Muon Solenoid (CMS) group, he’s part of a particle physics kinship that marked both loss and celebration during the week-long gathering.

A special memorial session honored Ian Shipsey, a foundational member of the community who passed away suddenly a month before the meeting. Among many contributions across the United States and Europe, Shipsey served as chair of the CMS experiment collaboration board, defined Fermilab’s Large Hadron Collider Physics Center, and was a founding chair of the CPAD organization—helping shape the scientific landscape students like Vendrasco are still exploring. 

The workshop also hailed the 50th anniversary of the Time Projection Chamber (TPC): physicist David Nygren’s innovative design to study tens of thousands of particles from a single collision event. A special plenary session included contributions from Nygren and leaders in the field who continue to use the TPC for discoveries today. A reception at the Sunsphere (with our own Bains Professor Steven Johnston signing on as DJ) was part of the celebration. Not to be outdone, Assistant Professor Larry Lee, Professor Norman Mannella, and local musician Dave Slack helped provide the musical backdrop for a closing banquet at the Knoxville Museum of Art.

Lee, who, like Holmes, invested hours of work in the event as part of the local organizing committee, had no doubts the effort was worth it.

“We were honored to host this important conference here on campus, bringing many of the world’s leaders in particle detection to Knoxville,” he said. “We had the opportunity to show the community the amazing research happening on campus and at ORNL, drive these historic special events, and plan for the future of particle physics. Not only did UT have a seat at the table; the table was in our living room.”

November 26, 2024  |  Filed Under: Featured News, News, Particle

A photo of Rebecca Godri at Oak Ridge National Laboratory

Another SCGSR Award for UT Physics

November 8, 2024

Rebecca Godri isn’t afraid of the hard work needed to test the Standard Model of Physics. As the department’s newest student selected for the prestigious Department of Energy (DOE) Office of Science Graduate Student Research (SCGSR) program, she’s won financial support to pursue this effort at Oak Ridge National Laboratory (ORNL).

Looking for new physics

As part of UT’s fundamental neutron physics group, Godri investigates the weak force, one of the four fundamental interactions in nature. She’s working on the Nab experiment at ORNL; a project designed to discover the nuances of neutron beta decay, a weak process.

A free (unbound) neutron is unstable: it will decay into a proton, electron, and antineutrino. Professor Nadia Fomin, one of Godri’s advisors, explained that “As experimentalists, we can ‘observe’ the neutron spin, momenta of the charged particles, and the angles between them. While the antineutrinos are detectable, the efficiency is very low, and we can get all the necessary information from basic principles of energy and momentum conservation.”

The Nab experiment will make precise determinations of “little a” and “little b,” decay correlation parameters of neutron beta decay. These determinations provide a stringent test for physics beyond the Standard Model.

Flipping the Spin

As small as protons, electrons, and antineutrinos are, the Nab experiment requires mighty tools to study them. Godri is working at the Fundamental Neutron Physics Beamline (FnPB) at the ORNL Spallation Neutron Source, a state-of-the-art facility that directs a powerful neutron stream down beamlines for instruments purpose-built for specific kinds of measurements. As their name implies, neutrons have no positive or negative charge. They do, however, have spin, a magnetic property that points them in certain direction. When neutrons decay, their speed, energy, and direction can give scientists critical information. The FnPB is unique in that can support different experiments with different full-scale apparatus, such as Nab.

Godri’s work, which she recently presented at an American Physical Society meeting, is getting neutrons to reveal more clues about the weak interaction in physics. To do that she’s measuring the residual polarization of the neutron beam at the FNPB and characterizing the Nab experiment’s spin flipper—a device that lets scientists control the neutron’s spin. She works with both Fomin at UT and Chenyang Jiang, a research scientist in ORNL’s Neutron Technologies Division.

While some may find all the preparation tedious, Godri said she enjoys both the groundwork and the payoff.

“The hands-on work is exciting,” she said. “My favorite part is being able to get data from the measurements we’ve spent months preparing for!”

An Easy Decision

Godri earned a bachelor’s degree in physics from the University of Tennessee at Chattanooga in 2021 and started her graduate studies in Knoxville that fall. She finished a master’s in physics last year and is working toward a PhD.

UT’s nuclear physics research opportunities made it an obvious choice for her graduate studies.

“Nadia’s research at ORNL aligned with my research interests post-undergrad, so UT was an easy decision,” she said. Godri’s SCGSR award is the 14th for UT Physics since 2016 and the fifth this year. She’s part of the latest cohort, comprising 62 PhD students from 24 states

A photo of Rebecca Godri at Oak Ridge National Laboratory
Rebecca Godri

November 8, 2024  |  Filed Under: Featured News, News, Nuclear

A photo of Tova Holmes

Cottrell Scholar Award for Tova Holmes

November 6, 2024

A photo of Tova Holmes
Tova Holmes

Tova Holmes is a big fan of tiny particles. She’d like it if you were too. An assistant professor of physics, she’s won a prestigious Cottrell Scholar Award to help her move physics forward while inspiring a larger cheering section for all science.

The Cottrell Scholar Awards recognize outstanding early-career teacher-scholars in chemistry, physics, and astronomy. Holmes is the first UT faculty member to win a Cottrell Award and one of 19 awardees in the 2024 cohort, each of whom receives $120,000 over three years. The goal is to support young scientists with innovative ideas who also have a gift for academic leadership. Each scholar writes a proposal for research and one for education. Holmes, who joined the faculty in 2020, is passionate about both. In 2023 UT’s physics majors selected her as their Research Advisor of the Year. As a Cottrell Scholar, she’ll teach students how to explain their work to a wide audience, as well as explore new ground for her own.

In the Room Where it Happened

In the early hours of July 4, 2012, Holmes, then a sleep-deprived graduate student, managed to get one of three remaining seats in the CERN auditorium to hear the official announcement that the Higgs boson had been discovered. The confirmation of this elusive particle, predicted 50 years earlier, completed the Standard Model of Physics. So on “Higgsdependence Day,” as she called it, Holmes was there, “at the center of discovery.” She was hooked.

Elementary particles are a bit like prime numbers. If you’re dividing a huge number, there comes a point where you can’t break it down any farther because the numbers left are indivisible. Atoms are sort of the same. Dividing an atom into its most minute components and figuring out how they work (or if there are more of them) takes scientists down to the bedrock of matter and tells them something about the universe, most of which is still a mystery. While the Standard Model organizes all the particles and forces governing matter, Holmes has set her sights on one: the muon.

Making Custom Particles

Digging down to matter’s foundations involves building high-energy colliders that accelerate beams of particles and then smash them together. Physicists wade through the aftermath, measuring the location and energies of known particles and looking for new ones. The Large Hadron Collider (LHC) at CERN has been remarkably successful at this, as evidenced by the Higgs discovery. But what comes next?

The LHC is a 27-kilometer underground ring crossing the French-Swiss border, hemmed in by mountains and Lake Geneva. To take the science farther and work at higher energies, the ring would have to be bigger. Holmes, however, is among the physicists who see energy, rather than real estate, as the solution. The muon is the key.

Muons are 200 times heavier than electrons and offer more energy for collisions. They also come with challenges. Particles in collision beams have to be aligned and headed in the same direction. For that to work, every collider up until now has used stable particles, like the protons at the LHC. Muons are more complicated. First, they have to be created by sending protons through a scientific obstacle course that begins with a linear accelerator and ultimately creates particles called pions, which decay into muons.

“They’re bespoke particles,” Holmes said. “You have to make them because they’re not sitting around. Then you have to deal with them in whatever state they’re in. (And) they only live about two microseconds.”

Before the muons decay, scientists have to compress them to fit into a beam, point them in the same direction, accelerate them, and finally collide them.

“That’s going to make things tricky,” Holmes said.

She’s is part of a growing group with a plan to navigate this tricky territory. Using magnets to collect the muons, they can slow them down by shooting them into a material, then accelerate them in one direction to align them. This is only one part of a muon collider, but by showing proof of principle, they move closer to making the technology a reality.

Their timing couldn’t be better.

The US particle physics community sees the muon collider as a centerpiece of the field’s future, as outlined in the scientific roadmap they announced last year. The Cottrell Award helps support Holmes’s postdocs and students so they can contribute to this work.

“What they’re currently doing is muddling their way through some pretty rough code that’s sort of been borrowed and adapted, and trying to squeeze information out of it about what kind of physics we can do,” she said. “We need to (make) that a more streamlined process. The proposal is really about engaging in that.”

Department Head Adrian Del Maestro said Holmes “is unique in her ability to inspire and challenge students to seek answers to some of the most fundamental problems in physics. She is an international leader in envisioning the future of the facilities needed to discover new particles, making the University of Tennessee a ‘theory of everything’ school.”

Getting the Message Across

Holmes’s students have joined a field that’s highly collaborative. She said creative thinking and effective communications are crucial in research areas like hers that involve thousands of scientists from across the world. Yet she’s seen that students typically don’t get the chance to develop those skills in the mainstream physics curriculum. Not only does this discourage students drawn to those ideas from majoring in physics, it also leaves physics graduates at a disadvantage.

“You’re not going to be good in my field if you can’t communicate to nearby experts,” she explained, adding that half of success in particle physics is explaining how what you learn is useful to others.

“(Communication) is not an afterthought: it’s a fundamental requirement,” she said. “My field’s not the only one that’s like that.”

Holmes was impressed by Professor David Matthew’s architecture and interior design students as she watched them brainstorm, refine, and work together to solve problems. She took notice of Senior Lecturer Sean Lindsay’s innovative course using science fiction to teach physics. Both also use a grading system outside the traditional instructor-assigned scores, encouraging students to self-assess and review one another’s work. She’s brought Matthews and Lindsay on board as collaborators as she uses her Cottrell Award to develop a special topics course.

Students will learn the basics of strong visual, written, and spoken communications. They’ll study design elements to make compelling graphics for their data and practice translating technical concepts into simpler language. Their final project will be convincing a non-scientist to see the value in science.

Holmes knows first-hand that discovery must be shared if it’s going to be appreciated. She’s been quoted in The New York Times, Nature, and Science about the possibility of a muon collider and what it means inside and outside the research community.

“If I want to get a multi-billion-dollar machine built in the US, I need to be able to communicate why that’s something that’s valuable to everybody in the US,” she said.

A Career Well Spent

Holmes is excited to broaden her own collaborations now that she’s part of the Cottrell Scholars community. Current and former scholars meet each year and build connections outside their typical research areas. While she has a scientist’s natural curiosity and open mind, her hope is that particle physics—driven by a new muon collider—will keep her occupied for the foreseeable future.

“That is my dream,” she said. “I think that would be a career well spent.”

November 6, 2024  |  Filed Under: Featured News, News, Particle

NOAA Geomagnetic Storm Alert October 2024

Aurora Alert!

October 10, 2024

From Paul Lewis, astronomy outreach director:

If you missed seeing the northern lights this spring, you have another chance!

The National Oceanic and Atmospheric Administration (NOAA) has issued a geomagnetic storm alert/watch for October 10-11. The storm watch is a G4, which means severe. There will be no observing from the Nielsen Physics Building roof those evenings, so take this opportunity to drive away from campus and city lights to try to see, if they actually appear, the northern lights or aurora.

Some of you may have been fortunate to see the spectacular display that occurred in May. There are certainly no guarantees for this, but if you don’t take the opportunity to look, you most certainly won’t see anything. 

Use your cellphone to try to get pictures, even if you can’t see the northern lights with the naked eye. The camera in your cellphone is more sensitive to the red and green light we usually see when there are bright aurorae. Look northwest to northeast for the best chance to see aurora. During the May storm we were able to see aurora to the south as well. That is rare here. Start looking as soon as it’s dark for at least a couple of hours.

There are several state parks nearby you might consider driving to. Look up Tennessee State Parks for more info and directions.

Good luck!

October 10, 2024  |  Filed Under: Astronomy, Featured News, News

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