New theoretical work shows how an unusual state of matter that oscillates between spin states could be used in timekeeping.
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The way you walk can reveal your true feelings
Whether you’re striding with purpose, swaggering with confidence, or trudging slowly along the street, the way you walk can reveal how you’re feeling, according to new research published in the journal Royal Society Open Science. We already know that some features of our gait can reflect our emotional state, such as heavy steps conveying anger and slumped shoulders indicating sadness. However, researchers led by Mina Wakabayashi at the Advanced Telecommunications Research Institute International in Japan and her colleagues sought to determine whether there is a specific, coordinated movement pattern that reliably signals these emotional states.
The team conducted two experiments. In the first, they asked actors to recall life events that evoked anger, happiness, fear, and sadness, and to then walk a short distance while contemplating each memory. The actors also walked with a neutral expression to give the researchers a baseline for comparison.
The recordings were then converted into point-light videos of 17 white dots representing the body’s main joints, which were shown to adult volunteers who had to click a button to identify the emotion they perceived. They correctly identified emotions at a level significantly above chance.
Superconductor advancement could unlock ultra-energy-efficient electronics
Superconducting materials could play a crucial role in the energy-efficient applications of the future. However, several technical challenges still stand in the way of their practical use. Now, researchers at Chalmers University of Technology in Sweden have developed a new material design that addresses a major obstacle in the field: enabling superconductivity to operate at higher temperatures while also withstanding strong magnetic fields. This breakthrough could pave the way for far more energy-efficient electronics and quantum technologies.
Digital devices, data centers and information and communications technology (ICT) networks currently account for approximately 6% to 12% of global electricity consumption. There is a substantial and growing need for more energy-efficient electronics and this is where superconducting materials have emerged as a promising solution. Unlike conventional electronics, which lose energy as heat, superconductors can conduct electricity with zero energy loss. Thus, superconductors have the potential to make power grids, electronics and quantum technologies hundreds of times more energy efficient.
However, the path to real-world applications is still blocked by several key challenges. One major obstacle is that superconducting states often require extremely low temperatures—down to around −200°C. Cooling to such temperatures is complex and energy-intensive. Another major challenge is that superconductivity can be weakened or destroyed by strong magnetic fields. This is a critical limitation, as magnetic fields are often present in advanced electronic devices and are essential to many quantum technologies.
Challenging a 300-year-old law of friction
Researchers at the University of Konstanz have uncovered a new mechanism of sliding friction: resistance to motion that arises without any mechanical contact, driven purely by collective magnetic dynamics. The study, published in Nature Materials, shows that friction does not necessarily increase steadily with load, as postulated by Amontons’ law—one of the oldest and most fundamental empirical laws of physics—but can instead exhibit a pronounced maximum when internal magnetic ordering becomes frustrated.
For more than three centuries, Amontons’ law has linked friction directly to load, reflecting the everyday experience that heavier objects are harder to move; for example, pushing a heavy piece of furniture requires far more effort than sliding a light chair. This behavior is commonly attributed to tiny deformations of the surfaces in contact under load, which increase the number of microscopic contact points and thereby enhance friction.
In most classical situations, these deformations remain small and do not qualitatively change the internal structure of the materials during sliding. It is therefore not clear whether Amontons’ law will also hold when sliding induces much stronger internal reconfigurations, as can occur in magnetic materials where motion can modify the magnetic order.
Terahertz spin waves can be converted into computer signals, study shows
What will the computers of tomorrow look like? Chances are good that spintronics will play a decisive role in the next generation of computers. In spintronics, the intrinsic angular momentum of an electron (the spin) is used to store, process and transmit data. This technology is already in use today, for example in hard drives. However, the scope of what is possible extends much further: More recent approaches aim at using not just individual spins, but entire spin waves made up of partly hundreds of trillions of spins. Such collective spin excitations are known as magnons. They could enable extremely energy-efficient data transmission—even in the terahertz range.
So far, so good. But how can these spin waves be coupled to today’s technology? “If we develop a concept to perform computer calculations with magnons, it must be compatible with the technology we currently use,” says physicist Davide Bossini from the University of Konstanz. “To reach this goal, you have to convert the spin wave into an electrical charge signal.” This spin-to-charge conversion is one of the major challenges of spintronics.
AI rebuilds molecules from exploding fragments
Researchers at the Department of Energy’s SLAC National Accelerator Laboratory and collaborating institutions recently built a generative AI model that can recreate molecular structures from the movement of the molecule’s ions after they are blasted apart by X-rays, a technique called Coulomb explosion imaging.
The research, published in Nature Communications, is an important step toward being able to take snapshots of molecules during chemical reactions—an advance that could have important impacts in medicine and industry. The machine learning model closely predicted the geometries of a range of different molecules made of less than ten atoms, paving the way for applying the technique to larger molecules.
“We were pretty excited about this,” said Xiang Li, an associate scientist at SLAC’s Linac Coherent Light Source (LCLS) and lead author of the study. “It is the first AI model built for molecular structure reconstruction from Coulomb explosion imaging.”
Clearest evidence yet that giant planets spin faster than their cosmic lookalikes
For decades, astronomers have struggled to differentiate giant planets from brown dwarfs, a class of objects more massive than planets but too small to ignite nuclear fusion like true stars. Through a telescope, these cosmic lookalikes can have overlapping brightness, temperatures, and even atmospheric fingerprints. The striking similarity leaves astronomers unsure if they have observed an oversized planet or an undersized star. Now, a Northwestern University-led team has uncovered a crucial clue that separates the two: how fast they spin.
In a new study, astrophysicists found the clearest evidence yet that giant planets spin significantly faster than their brown dwarf counterparts. The new results suggest rotation measurements may provide a powerful new diagnostic for classifying these indistinguishable populations and suggest that these two objects evolve differently, perhaps even forming through distinct processes.
The study was published in The Astronomical Journal. It marks the largest survey of spin measurements of directly imaged extrasolar planets and brown dwarfs to date.
How two dim stars came together to shine brightly
Brown dwarfs get a bad rap in the stellar world, often labeled as “failed stars” for their inability to sustain nuclear fusion at their cores. The mass of these objects falls between planets and stars, ranging from 13 to 80 times the mass of Jupiter. Because they aren’t massive enough to sustain fusion, they are far fainter and cooler than their stellar comrades.
Now, a new finding led by researchers at Caltech shows how these dim bulbs can join together to shine brightly. Searching through archival observations captured by the Zwicky Transient Facility (ZTF) at Caltech’s Palomar Observatory, researchers have identified a very tight-knit pair of brown dwarfs in which one is actively siphoning material from the other.
Ultimately, the brown dwarfs are expected to merge to form a new star; alternatively, the brown dwarf gaining the extra mass will ignite to become a star. Either way, a pair of failed stars will have created a brilliant new star.
Large-scale look at the exposome shows combined environmental exposures rival genetics in shaping human health outcomes
For decades, scientists have been carefully unraveling the role of genes in disease by examining how small variations in a person’s genetic code can shape lifelong risk of developing common conditions such as cancer, diabetes, or heart disease. But genetics only tell part of the story.
The other part comes from all the external and internal exposures a person experiences during their lifetime, which can range from pollution to infections to diet and lifestyle. Cumulatively, these exposures—and the body’s biological response to them—make up what scientists have termed the exposome.
A team led by scientists at Harvard Medical School has now conducted what may be the largest-scale study to date to quantify the relationships between exposures and health outcomes, testing more than 100,000 associations. The work demonstrates the importance of studying potential environmental disease risks in aggregate rather than one at a time.
NASA’s Hubble unexpectedly catches comet breaking up
In a happy twist of fate, NASA’s Hubble Space Telescope witnessed a comet in the act of breaking apart. The chance of that happening while Hubble watched is extraordinarily minuscule. The findings are published in the journal Icarus.
The comet K1, whose full name is C/2025 K1 (ATLAS)—not to be confused with interstellar comet 3I/ATLAS—was not the original target of the Hubble study.
“Sometimes the best science happens by accident,” said co-investigator John Noonan, a research professor in the Department of Physics at Auburn University in Alabama. “This comet got observed because our original comet was not viewable due to some new technical constraints after we won our proposal. We had to find a new target—and right when we observed it, it happened to break apart, which is the slimmest of slim chances.”