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Scientist captures tiny particles for clues on what sparks lightning

Using lasers as tweezers to understand cloud electrification might sound like science fiction, but at the Institute of Science and Technology Austria (ISTA) it is a reality. By trapping and charging micron-sized particles with lasers, researchers can now observe their charging and discharging dynamics over time.

This method, published in Physical Review Letters, could provide key insights into what sparks lightning.

Aerosols are liquid or that float in the air. They are all around us. Some are large and visible, such as pollen in spring, while others, such as viruses that spread during flu season, cannot be detected by the naked eye. Some we can even taste, like the airborne salt crystals we breathe in at the seaside.

Coaxing bilayer graphene into a single diamond-like layer for industrial applications

Graphene’s enduring appeal lies in its remarkable combination of lightness, flexibility, and strength. Now, researchers have shown that under pressure, it can briefly take on the traits of one of its more glamorous carbon cousins.

By introducing nitrogen atoms and applying pressure, a team of scientists has coaxed bilayer grown through chemical vapor deposition (CVD) into a diamond-like phase—without the need for extreme heat. The finding, reported in Advanced Materials Technologies, shows a scalable way to create ultrathin coatings that combine the toughness of diamond with the processability of graphene.

When superfluids collide, physicists find a mix of old and new behavior

Physics is often about recognizing patterns, sometimes repeated across vastly different scales. For instance, moons orbit planets in the same way planets orbit stars, which in turn orbit the center of a galaxy.

When researchers first studied the structure of atoms, they were tempted to extend this pattern down to smaller scales and describe electrons as orbiting the nuclei of atoms. This is true to an extent, but the quirks of quantum physics mean that the pattern breaks in significant ways. An electron remains in a defined orbital area around the nucleus, but unlike a classical orbit, an electron will be found at a random location in the area instead of proceeding along a precisely predictable path.

That electron orbits bear any similarity to the orbits of moons or planets is because all of these orbital systems feature attractive forces that pull the objects together. But a discrepancy arises for electrons because of their .

Surface-only superconductor is the strangest of its kind

Something strange goes on inside the material platinum-bismuth-two (PtBi₂). A new study by researchers at IFW Dresden and the Cluster of Excellence ct.qmat demonstrates that while PtBi₂ may look like a typical shiny gray crystal, electrons moving through it do some things never seen before.

In 2024, the research team demonstrated that the top and bottom surfaces of the material superconduct, meaning pair up and move without resistance.

Now, they reveal that this pairing works differently from any superconductor we have seen before. Enticingly, the edges around the superconducting surfaces hold long-sought-after Majorana particles, which may be used as fault-tolerant quantum bits (qubits) in quantum computers.

JUNO experiment delivers first physics results two months after completion

The Institute of High Energy Physics (IHEP) of the Chinese Academy of Sciences has successfully completed the Jiangmen Underground Neutrino Observatory (JUNO) and released its first physics results.

After more than a decade of design, construction, and international collaboration, JUNO has become the world’s first next-generation, large-scale, high-precision neutrino detector to begin operation.

Early data show that the detector’s key performance indicators fully meet or surpass design expectations, confirming that JUNO is ready to deliver frontier measurements in neutrino physics.

Cosmic Paradox Reveals the Awful Consequence of an Observer-Free Universe

From the article:

Quantum mechanics requires a distinction between an observer — such as the scientist carrying out an experiment — and the system they observe. The system tends to be something small and quantum, like an atom. The observer is big and far away, and thus well described by classical physics. Shaghoulian observed that this split was analogous to the kind that enlarges the Hilbert spaces of topological field theories. Perhaps an observer could do the same to these closed, impossibly simple-seeming universes?

In 2024, Zhao moved to the Massachusetts Institute of Technology, where she began to work on the problem of how to put an observer into a closed universe. She and two colleagues —Daniel Harlow and Mykhaylo Usatyuk — thought of the observer as introducing a new kind of boundary: not the edge of the universe, but the boundary of the observer themself. When you consider a classical observer inside a closed universe, all the complexity of the world returns, Zhao and her collaborators showed.

The MIT team’s paper(opens a new tab) came out at the beginning of 2025, around the same time that another group came forward with a similar idea(opens a new tab). Others chimed in(opens a new tab) to point out connections to earlier work.

At this stage, everyone involved emphasizes that they don’t know the full solution. The paradox itself may be a misunderstanding, one that evaporates with a new argument. But so far, adding an observer to the closed universe and trying to account for their presence may be the safest path.

“Am I really confident to say that it’s right, it’s the thing that solves the problem? I cannot say that. We try our best,” Zhao said.

If the idea holds up, using the subjective nature of the observer as a way to account for the complexity of the universe would represent a paradigm shift in physics. Physicists typically seek a view from nowhere, a stand-alone description of nature. They want to know how the world works, and how observers like us emerge as parts of the world. But as physicists come to understand closed universes in terms of private boundaries around private observers, this view from nowhere seems less and less viable. Perhaps views from somewhere are all that we can ever have.

Physicists demonstrate the constancy of the speed of light with unprecedented accuracy

In 1887, one of the most important experiments in the history of physics took place. American scientists Michelson and Morley failed to measure the speed of Earth by comparing the speed of light in the direction of Earth’s motion with that perpendicular to it. That arguably most important zero measurement in the history of science led Einstein to postulate that the speed of light is constant and consequently to formulate his theory of special relativity.

This theory implies that all laws of physics are the same, independent of the relative motion between observers—a concept known as Lorentz invariance.

Meanwhile, has been developed, with Lorentz invariance at the heart of all its theoretical frameworks, in particular quantum field theory and the Standard Model of Particle Physics. The latter is the most precisely tested theory ever developed and has been verified to incredible precision.

New magnetic component discovered in the Faraday effect after nearly two centuries

Researchers at the Hebrew University of Jerusalem discovered that the magnetic component of light plays a direct role in the Faraday effect, overturning a 180-year-old assumption that only its electric field mattered.

Their findings, published in Scientific Reports, show that light can magnetically influence matter, not just illuminate it. The discovery opens new possibilities in optics, spintronics, and quantum technologies.

The study was led by Dr. Amir Capua and Benjamin Assouline from the Institute of Electrical Engineering and Applied Physics at the Hebrew University of Jerusalem. It presents the first theoretical proof that the oscillating of light directly contributes to the Faraday effect, a phenomenon in which the polarization of light rotates as it passes through a material exposed to a constant magnetic field.

Electroexcitation of Nucleon Resonances and Emergence of Hadron Mass

Developing an understanding of phenomena driven by the emergence of hadron mass (EHM) is one of the most challenging problems in the Standard Model. This discussion focuses on the impact of results on nucleon resonance (N electroexcitation amplitudes (or γvpN* electrocouplings) obtained from experiments during the 6 GeV era in Hall B at Jefferson Lab on understanding EHM. Analyzed using continuum Schwinger function methods (CSMs), these results have revealed new pathways for the elucidation of EHM. A good description of the Δ(1232)3/2+, N(1440)1/2+, and Δ(1600)3/2+ electrocouplings, achieved by CSM analyses that express a realistic dressed quark mass function, sheds light on the strong interaction dynamics underlying EHM. Extensions to N* studies for higher-mass states are outlined, as well as experimental results anticipated in the 12 GeV era at Jefferson Lab and those that would be enabled by a further increase in the beam energy to 22 GeV.

Supercomputer Models Revise Enceladus Ice Loss

“The mass flow rates from Enceladus are between 20 to 40 percent lower than what you find in the scientific literature,” said Dr. Arnaud Mahieux.


How much ice is Saturn’s moon, Enceladus, losing to space when it discharges its interior ocean? This is what a recent study published in the Journal of Geophysical Research: Planets hopes to address as a team of scientists investigated whether Enceladus’ plume environments, including discharge rates, temperatures, and ice particle sizes could be determined strictly from observational data. This study has the potential to help scientists develop new methods for exploring icy bodies, especially those like Enceladus that could harbor life within its liquid water ocean.

For the study, the researchers used a series of computer models to analyze data obtained from NASA’s now-retired Cassini spacecraft, which intentionally burned up in Saturn’s atmosphere in 2017 after running low on fuel. This was done to avoid potentially contaminating moons like Enceladus with microbes from Earth and interfere with potential life there. During its journey at Saturn and its many moons, Cassino both discovered and flew through the plumes of Enceladus, which are at the moon’s south pole and emit large quantities of water ice and other substances into space from its subsurface liquid water ocean. It’s the amount of water and ice these plumes discharge that have intrigued scientists, and the results were surprising.

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