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Tokamak regime sustains stable fusion plasma for one minute while easing heat loads

For the first time, a research team has demonstrated, in a metal-wall environment, a plasma regime that simultaneously achieves partial divertor detachment, an edge-localized-mode (ELM)-free high-confinement mode (H-mode), and high pedestal performance. This integrated regime was sustained on a minute scale and the work is published in Physical Review Letters.

The team was led by Professor Xu Guosheng from the Institute of Plasma Physics, Hefei Institutes of Physical Science, Chinese Academy of Sciences.

Controllable nuclear fusion requires managing extreme heat loads on divertor plates while maintaining plasma stability. While impurity gases can reduce divertor heat through detachment, excessive cooling can damage the plasma edge, and H-mode plasmas are prone to sudden, damaging ELMs. Achieving a steady-state regime that addresses both challenges has been a major international goal.

Netta Engelhardt: Puzzles in the Black Hole Interior: Past, Present and Future (April 22, 2026)

In this Presidential Lecture, Netta Engelhardt will (metaphorically!) dive straight into the black hole interior to explain the origin of this puzzle and its significance in modern physics. The lecture will then turn to the recent revolution in physicists’ understanding of the black hole information paradox and the current state of the resolution. She will conclude with a discussion of where these new insights may lead, what questions remain outstanding and how this may all fit into the universe at large.

Astronomers Find the Edge of the Milky Way’s Star-Forming Disc

Where exactly is the edge of the Milky Way? That question is harder to answer than one might expect. Since we’re inside of the galaxy itself, it’s obviously hard to judge the “edge” to begin with. But it gets even more complicated when defining what the edge even is — the galaxy simply gets less dense the farther away from the center it goes. A new paper by researchers originally at the University of Malta thinks they have an answer though. The “edge” can be defined as the star-forming region, and in their paper, published in Astronomy & Astrophysics, they very clearly show that “edge” to be between 11.28 and 12.15 kiloparsecs (or about 40,000 light years) from the center.

Even finding that edge was no easy task, though. The researchers had to analyze the ages of over 100,000 giant stars from the data of several different surveys, including APOGEE-DR17, LAMOST-DR3 and Gaia. In the data they found an interesting story about the evolution of the position of stars in the galaxy, and their age.

That relationship can be thought of as a U curve. In this case, the Y axis is age, and the X axis is the distance from the galaxy’s center. A picture (or graph in this case) is worth a thousand words, but in words that simply means that stars closer to the center of the galaxy are older, and get progressively younger out to a certain point, and then start getting older again. That “certain point”, according to the authors, is the end of the galaxy’s star-forming region, and hence, the “edge” of the galaxy.

The Space Habitat Diaspora — Humanity Spreads Without Planets

Humanity may not colonize planets—we may build our own worlds. Explore how rotating space habitats could spread across the Solar System and beyond, forming a vast diaspora of artificial worlds that reshape civilization and interstellar expansion.

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Watch my exclusive video Settling Saturn’s Rings: https://nebula.tv/videos/isaacarthur–… SFIA Merchandise: https://isaac-arthur-shop.fourthwall… 🌐 Visit our Website: http://www.isaacarthur.net ❤️ Support us on Patreon: / isaacarthur ⭐ Support us on Subscribestar: https://www.subscribestar.com/isaac-a… 👥 Facebook Group: / 1,583,992,725,237,264 📣 Reddit Community: / isaacarthur 🐦 Follow on Twitter / X: / isaac_a_arthur 💬 SFIA Discord Server: / discord Credits: The Space Habitat Diaspora – Humanity Spreads Without Planets Written, Produced & Narrated by: Isaac Arthur Graphics from Bryan Versteeg, Jeremy Jozwik, Sergio Botero, Udo Schroeter Select imagery/video supplied by Getty Images 0:00 Intro — Rethinking What a World Can Be 2:37 Why Habitats Win on Physics, Engineering… and Scalability 10:13 The Birth of a Habitat Civilization 14:54 Nebula 15:54 Life Without Planets: Cultures That Grow in Steel Valleys 18:59 Resilience: Fragile Shells, Immortal Civilizations 21:37 The True Diaspora: Leaving the Solar System.

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Credits:
The Space Habitat Diaspora – Humanity Spreads Without Planets.
Written, Produced & Narrated by: Isaac Arthur.
Graphics from Bryan Versteeg, Jeremy Jozwik, Sergio Botero, Udo Schroeter.
Select imagery/video supplied by Getty Images.

0:00 Intro — Rethinking What a World Can Be.
2:37 Why Habitats Win on Physics, Engineering… and Scalability.
10:13 The Birth of a Habitat Civilization.
14:54 Nebula.
15:54 Life Without Planets: Cultures That Grow in Steel Valleys.
18:59 Resilience: Fragile Shells, Immortal Civilizations.
21:37 The True Diaspora: Leaving the Solar System.

Breaking connections helps ideas spread farther, says physics-based study

Sticking with the same people might feel safe and comfortable. But a new Northwestern University study suggests it can actually trap new ideas and behaviors inside tight echo chambers. By contrast, the research, published in Communications Physics, shows that when interactions shift away from familiar contacts—and toward new ones—activity can spread more widely.

To explore how activities spread across networks, physicists developed a new theoretical framework that includes simple “learning” rules. While traditional network models assume relationships do not change, the new model shows what happens when connections change with experience. As interactions strengthen or weaken relationships, they gradually reshape the entire network.

The findings apply not only to ideas moving through social networks but to a wide range of systems where activity spreads, including infections passing among people, signals traveling through the brain and behaviors proliferating through groups of animals. Ultimately, the study suggests that whether something spreads or stalls may hinge on a simple choice: revisit the same connections or explore new ones.

Neural network speeds tuning of attosecond light pulses for physics experiments

Researchers from Skoltech and the Shanghai Institute of Optics and Fine Mechanics have developed an approach that helps optimize the parameters of a laser-plasma source of attosecond pulses—ultrashort flashes of light used in physics experiments. Instead of relying on a large number of time-consuming calculations, the team trained a neural network to quickly identify promising settings and thereby speed up the optimization of the sophisticated laboratory equipment.

The results were published in Communications in Nonlinear Science and Numerical Simulation.

Attosecond pulse sources are used as research tools. They are applied in ultrafast spectroscopy, studies of magnetic materials, chiral molecules, and electron dynamics in matter. The goal of this work is to make it faster to tune a light source with the required properties for such experiments.

Self-regulating process governs cosmic order inside star clusters

A team of astrophysicists from Nanjing University and University of Bonn have demonstrated that, rather than being random, the mass of new stars born inside a star cluster is actually governed by a defined process of self-regulation. Their work has been published in the journal Research in Astronomy and Astrophysics.

When a galaxy welcomes new stars, they are usually formed in star clusters inside vast gas clouds. While some of these stars inside such clusters are small, cool and dim, others possess 10 times the mass of our sun and a hundred thousand times higher brightness—but also a shorter lifespan as a result. These differences in initial mass have a significant influence on a galaxy’s luminosity.

“The total mass of a dwarf galaxy is relatively low, so it won’t produce any extremely massive stars that’d be brighter than our sun,” explains Professor Pavel Kroupa from the Helmholtz Institute for Radiation and Nuclear Physics at the University of Bonn. “By contrast, very massive elliptical galaxies, which formed almost 10 billion stars in just 10 million years during the early stage of the universe, generate millions of these ultra-bright stars.”

Experimental Evidence That Universe Could Just Vanish One Day

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Hello and welcome! My name is Anton and in this video, we will talk about a false vacuum experiment that shows us one day the universe could just vanish
Links:
https://arxiv.org/pdf/2512.04637
Previous video: • Experimental Evidence of a Phenomenon That…
#falsevacuum #physics #science.

0:00 Can universe just kind of end?
1:10 New study and an experiment
2:08 What is false vacuum?
4:35 True vacuum transition
5:30 What would happen to the universe?
6:20 Experimental system and a molecular analog
8:10 Previous experiments and achievements
9:30 Explanation the inflation
10:20 Should we be worried?
11:35 Implications for physics.

Enjoy and please subscribe.

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Cell membranes may store memories after electrical stimulation

The science of memories has been pursued and studied since the days of ancient Greece and Aristotle. Today, research conducted by Dima Bolmatov, assistant professor in the Department of Physics & Astronomy at Texas Tech University, is considering how memories are stored on a cellular level.

Bolmatov’s research centers on lipid bilayers, membranes that serve as a continuous barrier around cells. These membranes, he noted, were traditionally viewed as passive barriers.

“I began to see that they behave more like dynamic, adaptive materials,” he stated. “They respond to electrical stimulation, retain history and exhibit collective behavior. This realization suggests that membranes themselves may participate in information processing, bridging physics and biology in a fundamentally new way.”

Our Universe Might Be a Giant Brain, According to New Theories

There’s something quietly unsettling about placing a photograph of a human neuron next to a simulated image of the large-scale cosmic web. The two look almost identical: delicate, branching filaments connecting dense clusters, with vast open spaces in between. One fits inside your skull. The other stretches across billions of light-years. The resemblance is hard to dismiss, and for a growing number of researchers, it’s far more than a visual coincidence.

What started as a striking observation in cosmology and neuroscience has evolved into a serious theoretical question. Could the universe, at its most fundamental level, operate the way a brain does? The ideas being put forward aren’t purely philosophical. Some of them come with testable mathematics, published peer-reviewed papers, and the names of well-regarded physicists attached. What follows is an honest look at where the science currently stands.

The estimated 200 billion detectable galaxies aren’t distributed randomly, but are lumped together by gravity into clusters that form even larger clusters, which are connected to one another by “galactic filaments,” long thin threads of galaxies. This vast architecture is what scientists call the cosmic web. When you zoom far enough out, the structure of the entire observable universe begins to take on a shape that looks startlingly familiar.

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