To request a media interview, please reach out to School of Physics experts using our faculty directory, or contact Jess Hunt-Ralston, College of Sciences communications director. A list of faculty experts and research areas across the College of Sciences at Georgia Tech is also available to journalists upon request.
Why was School of Biological Sciences associate professor David Hu drawn towards mammal poop as the topic of a new study? His experience as a working dad, he recently posted on the Conversation blog, "turned me from a poo-analysis novice to a wizened connoisseur." The people running the PBS Newshour website had a chance to digest the post and decided to share it in full on their Rundown blog. Hu is also a adjunct associate professor in the School of Physics and an associate professor in the George W. Woodruff School of Mechanical Engineering. Patricia Yang, a Ph.D. student in the Woodruff School of Mechanical Engineering, co-authored the study, which appeared in Soft Matter.
Faculty-Led Study Abroad Programs 2017-04-27T00:00:00-04:00Everyone poops, and it takes them about the same amount of time. A new study of the hydrodynamics of defecation finds that all mammals take 12 seconds on average to relieve themselves, no matter how large or small the animal. The research, published in Soft Matter, reveals that the soft matter coming out of the hind ends of elephants, pandas, warthogs and dogs slides out of the rectum on a layer of mucus that keeps toilet time to a minimum. “The smell of body waste attracts predators, which is dangerous for animals. If they stay longer doing their thing, they’re exposing themselves and risking being discovered,” says Patricia Yang, a mechanical engineer at the Georgia Institute of Technology in Atlanta. Yang, a doctoral student in the Woodruff School of Mechanical Engineering, worked on the study with David Hu, associate professor in the School of Biological Sciences and an adjunct associate professor in the School of Physics.
All mammals big or small take about 12 seconds to defecate 2017-04-26T00:00:00-04:00Somebody give David Hu's graduate and undergraduate students medals for bravery -- and maybe some hazmat suits. Hu, an associate professor in the School of Biological Sciences and an adjunct associate professor in the School of Physics, is a 2015 Ig Nobel Prize winner for his "urination duration" research, and he and his intrepid fluid dynamics team have also gotten hands-on (yuck) with frog saliva. Now he has studied the physics of poop among mammals, venturing to Zoo Atlanta to follow elephants around and figure out things like speed, duration, size, mucosity, etc. Hu, also an associate professor in the George W. Woodruff School of Mechanical Engineering, makes the connection between his research and a better understanding of gastrointestinal health. The research also helped his team design state-of-the-art undergarments for astronauts. Hu's study was published April 25 in the journal (wait for it)....Soft Matter.
extreme temperatures 2017-04-26T00:00:00-04:00Imagine a liquid that could move on its own without human effort or the pull of gravity. You could put it in a container flat on a table, not touch it in any way, and it would still flow. As reported in Science, researchers have taken the first step in creating a self-propelling liquid. The finding offers the promise of developing an entirely new class of fluids that can flow without human or mechanical effort. School of Physics Associate Professor Alberto Fernandez-Nieves and postdoctoral fellow Ya-Wen Chang co-authored the study, which was led by collaborators at Brandeis University.
reconfigurable transceivers 2017-03-28T00:00:00-04:00To explore the mathematical possibilities of alternative geometries, mathematicians imagine such ‘non-Euclidean’ spaces, where parallel lines can intersect or veer apart. Now, with the help of relatively affordable VR devices, researchers are making curved spaces — a counter-intuitive concept with implications for Einstein’s theory underlying gravity and also for seismology — more accessible. They may even uncover new mathematics in the process. “You can think about it, but you don’t get a very visceral sense of this until you actually experience it,” says Elisabetta Matsumoto, a physicist at the Georgia Institute of Technology in Atlanta.
college of engineering; ISyE; fellowships; grad students; student awards; orise; cdc 2017-03-21T00:00:00-04:00Bright radiation emitted by neighboring galaxies likely fueled the rapid growth of supermassive black holes in the early universe, a new study shows. John Wise, an associate professor in the School of Physics, is a co-author of the study.
GradIO 2017-03-18T00:00:00-04:00It’s no secret that supermassive black holes are heartless beasts: These objects of immense gravity that let nothing, not even light escape, have fascinated astronomers since the early 20th century. While it’s believed that so-called supermassive black holes lurk at the center of most galaxies, including our own, there’s still much we don’t know about how they formed, or why, except to remind us of our own mortality. But new research from an international team of scientists might have some answers to at least one of the critical questions -- namely, how supermassive black holes, which range in size from millions to billions of solar masses, apparently formed very quickly in the early universe. Using computer simulations, the researchers found that these giants can grow incredibly fast if they can suck the life (read: radiation) out of a nearby galaxy, disabling their host galaxy’s ability to create stars...The researchers found that the neighboring galaxy supplying the radiation had to be a certain size and distance away from the black hole’s host galaxy -- though these cosmic energy sources could be smaller and closer galaxies than other studies estimated. “The nearby galaxy can’t be too close, or too far away, and like the Goldilocks principle, too hot or too cold,” study co-author John Wise, an associate astrophysics professor at Georgia Tech, said. Wise is an associate professor in the School of Physics.
faculty spotlight 2017-03-13T00:00:00-04:00
More than ten years ago, astronomers made a discovery that has puzzled them ever since – supermassive black holes appeared to have popped up soon after the start of the Universe. It is thought to take billions of years for supermassive black holes to form, but at least 20 of them were spotted at the dawn of the Universe, just 800 million years after the Big Bang. A team of researchers from Dublin City University, Columbia University, Georgia Tech, and the University of Helsinki, have now used computer simulations to attempt to solve the mystery. The results say a black hole can grow quickly if the galaxy it is in stops forming stars....To stop stars forming, there has to be a bright galaxy nearby, emitting radiation that can split molecular hydrogen into atomic hydrogen. This prevents stars in the galaxy from forming from the molecular hydrogen...."The nearby galaxy can't be too close, or too far away, and like the Goldilocks principle, too hot or too cold," said co-author John Wise, from Georgia Tech. The researchers published their findings in Nature Astronomy. John Wise is an associate professor in the School of Physics.
in solidarity 2017-03-13T00:00:00-04:00New research clarifies how toroidal droplets—which initially take the shape of a donut—evolve into spherical droplets by collapsing into themselves or breaking up into smaller droplets. Work with droplets has implications for the life sciences, and could improve industrial processes....“Surface tension drives the evolution of the droplets,” says Alexandros Fragkopoulos, a PhD candidate at Georgia Institute of Technology. “Fluids tend to minimize their surface area for a given volume because that minimizes the energy required to have an interface between different fluids. Spherical shapes minimize that energy, and as a result, toroidal droplets want to evolve to become spherical. We’re studying how that transition occurs."...The impetus for the experimental work was inconsistencies between theoretical predictions and computer simulation of toroidal droplet transitions. What the researchers found tends to back up the simulation results. “However, the earlier theoretical work was essential in guiding the theory efforts and in illustrating what the problem was in order to correctly describe the experimental results,” says Alberto Fernandez-Nieves, in whose lab the research took place. Alexandros Fragkopoulos is a graduate teaching assistant in the School of Physics, where Alberto Fernandez-Nieves is an associate professor.
reconfigurable transceivers 2017-03-13T00:00:00-04:00Supermassive black holes sit at the center of nearly every massive galaxy situated in the universe. Scientists don’t know how supermassive black holes form, but a new paper in the journal Nature Astronomy, illustrates a theory crazy enough to perhaps work. The running hypothesis is that black holes are born out of the collapse of a star, which can eventually suck up enough mass that they grow into supermassive black holes (SBHs). That process is thought to take billions of years, but scientists have already catalogued some SBHs that date back to 13.8 billion years in age — also the age of the universe. This would mean that some SBHs, if not all, form much more quickly than scientists originally suspected...If a huge nearby galaxy could pump enough radiation into a smaller galaxy that already hosted a black hole, the radiation could split molecular hydrogen into atomic hydrogen, stopping the galaxy from forming new stars and ultimately forcing it to collapse under the gravitational pressure of the black hole. Thus, the black hole would suck up that mass and quickly become an SBH...“The nearby galaxy can’t be too close, or too far away, and like the Goldilocks principle, too hot or too cold,” said John Wise, co-author of the study and associate astrophysics professor at Georgia Tech. Wise is an associate professor in the School of Physics.
Murder Mystery 2017-03-13T00:00:00-04:00You never know when a frog playing an electronic game will lead to an experiment on the physics of saliva....Alexis C. Noel, a Ph.D. student in mechanical engineering at Georgia Tech, and her supervisor, David L. Hu, were watching a viral YouTube video in which a frog is attacking the screen of a smartphone running an ant-smashing game. It appears to be winning. They started wondering how — in reality — frog tongues stick to insects so quickly when they shoot out to grab them, and decided it was a phenomenon worth studying. David Hu is an associate professor of mechanical engineering and of biology, as well as an adjunct associate professor of physics, at Georgia Tech.
Extension of Self 2017-02-06T00:00:00-05:00Georgia Tech researchers explain how frogs maintain their grip on their prey during the speedy attacks with their prehensile tongues. The study, published in the Journal of the Royal Society Interface, was conducted by mechanical engineering Ph.D. student Alexis Noel under the guidance of David Hu, a professor of mechanical engineering and of biology and an adjunct professor of physics.
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Events
FulminoSat: Using Lightning to Measure the Ionosphere with a Georgia Tech CubeSat Constellation
Learn how Georgia Tech researchers are leveraging lightning and CubeSat technology to study space weather and its impacts on critical space‑enabled systems.
School of Physics Spring Colloquium Series- Dr. Konrad Lehnert
Dr. Konrad Lehnert(Yale) Building quantum technology from quantum sound
College of Sciences Town Hall
College of Sciences students, faculty, and staff are invited to our end-of-school year town hall.
Experts in the News
Research led by Georgia Tech physicist Itamar Kolvin has found that the presence of small imperfections or heterogeneities in materials can have a dual effect on their strength and resilience. While heterogeneities were historically believed to make materials stronger by creating an obstacle course for cracks, the new study shows that in some complex materials, heterogeneities can actually accelerate crack propagation and weaken the overall structure. The findings have implications for how engineers design and reinforce materials to optimize their toughness.
Atlanta Today 2026-02-27T00:00:00-05:00Assistant Professor Zhu-Xi Luo and Ph.D. student Yi-Lin Tsao from Georgia Institute of Technology's School of Physics have demonstrated a novel mechanism for stabilising physical phases vulnerable to topological defects. Their work addresses a fundamental problem in condensed matter physics: the destabilisation of phases like superfluids by thermally-induced defects such as anyons and vortices.
Quantum Zeitgeist 2026-02-25T00:00:00-05:00In an article published in Physics Magazine, School of Physics Ph.D. student Jingcheng Zhou and Assistant Professor Chunhui (Rita) Du review efforts to optimize diamond-based quantum sensing. According to Zhou and Du, the approach used in two recent studies broadens the potential applications of nitrogen-vacancy center sensors for probing quantum phenomena, enabling measurements of nonlocal properties (such as spatial and temporal correlations) that are relevant to condensed-matter physics and materials science.
Physics Magazine 2025-07-14T00:00:00-04:00Researchers at the Georgia Institute of Technology and India's National Center for Biological Sciences have found that yeast clusters, when grown beyond a certain size, spontaneously generate fluid flows powerful enough to ferry nutrients deep into their interior.
In the study, "Metabolically driven flows enable exponential growth in macroscopic multicellular yeast," published in Science Advances, the research team — which included Georgia Tech Ph.D. scholar Emma Bingham, Research Scientist G. Ozan Bozdag, Associate Professor William C. Ratcliff, and Associate Professor Peter Yunker — used experimental evolution to determine whether non-genetic physical processes can enable nutrient transport in multicellular yeast lacking evolved transport adaptations.
A similar story also appeared at The Hindu.
Phys.org 2025-06-24T00:00:00-04:00Other planets, dwarf planets and moons in our solar system have seasonal cycles — and they can look wildly different from the ones we experience on Earth, experts told Live Science.
To understand how other planets have seasons, we can look at what drives seasonal changes on our planet. "The Earth has its four seasons because of the spin axis tilt," Gongjie Li, associate professor in the School of Physics, told Live Science. This means that our planet rotates at a slight angle of around 23.5 degrees.
"On Earth, we're very lucky, this spin axis is quite stable," Li said. Due to this, we've had relatively stable seasonal cycles that have persisted for millennia, although the broader climate sometimes shifts as the entire orbit of Earth drifts further or closer from the sun.
Such stability has likely helped life as we know it develop here, Li said. Scientists like her are now studying planetary conditions and seasonal changes on exoplanets to see whether life could exist in faroff worlds. For now, it seems as though the mild seasonal changes and stable spin tilts on Earth are unique.
Live Science 2025-05-05T00:00:00-04:00Biofilms have emergent properties: traits that appear only when a system of individual items interacts. It was this emergence that attracted School of Physics Associate Professor Peter Yunker to the microbial structures. Trained in soft matter physics — the study of materials that can be structurally altered — he is interested in understanding how the interactions between individual bacteria result in the higher-order structure of a biofilm
Recently, in his lab at the Georgia Institute of Technology, Yunker and his team created detailed topographical maps of the three-dimensional surface of a growing biofilm. These measurements allowed them to study how a biofilm’s shape emerges from millions of infinitesimal interactions among component bacteria and their environment. In 2024 in Nature Physics, they described the biophysical laws that control the complex aggregation of bacterial cells.
The work is important, Yunker said, not only because it can help explain the staggering diversity of one of the planet’s most common life forms, but also because it may evoke life’s first, hesitant steps toward multicellularity.
Quanta Magazine 2025-04-21T00:00:00-04:00