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Category: particle physics

A large team of researchers working on the Alpha Magnetic Spectrometer Collaboration, which has been analyzing eleven years’ worth of data from the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station, has found trends in the number of particles moving around in the heliosphere and in the way they interact with one another.

The team has published two papers in the journal Physical Review Letters; one describing trends they found surrounding antiproton and elementary particle behavior over a single and the other covering solar modulation of cosmic nuclei behavior, also over a single solar cycle.

Prior research has shown that the sun follows a cycle that repeats itself every 11 years. The AMS has been running for more than 11 years, but the researchers working on both efforts focused on conditions during just one cycle. They wanted to know how the sun impacted energy particles in the and beyond.

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Can copper be turned into gold? For centuries, alchemists pursued this dream, unaware that such a transformation requires a nuclear reaction. In contrast, graphite—the material found in pencil tips—and diamond are both composed entirely of carbon atoms; the key difference lies in how these atoms are arranged. Converting graphite into diamond requires extreme temperatures and pressures to break and reform chemical bonds, making the process impractical.

A more feasible transformation, according to Prof. Moshe Ben Shalom, head of the Quantum Layered Matter Group at Tel Aviv University, involves reconfiguring the atomic layers of graphite by shifting them against relatively weak van der Waals forces. This study, led by Prof. Ben Shalom and Ph.D. students Maayan Vizner Stern and Simon Salleh Atri, all from the Raymond & Beverly Sackler School of Physics & Astronomy at Tel Aviv University, was recently published in the journal Nature Review Physics.

While this method won’t create diamonds, if the switching process is fast and efficient enough, it could serve as a tiny electronic memory unit. In this case, the value of these newly engineered “polytype” materials could surpass that of both diamonds and gold.

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Quantum spin liquids (QSLs) are fascinating and mysterious states of matter that have intrigued scientists for decades. First proposed by Nobel laureate Philip Anderson in the 1970s, these materials break the conventional rules of magnetism by never settling into a stable magnetic state, even at temperatures close to absolute zero.

Instead, the spins of the atoms within them remain constantly fluctuating and entangled, creating a kind of magnetic “liquid.” This unusual behavior is driven by a phenomenon called magnetic frustration, where competing forces prevent the system from reaching a single, ordered configuration.

QSLs are notoriously difficult to study. Unlike ordinary magnetic materials, they don’t show the usual signs of magnetic transitions, which makes it hard to detect and understand them using traditional techniques. As a result, their behavior has remained an elusive puzzle for researchers.

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Whether you’re a surly gang of bosons or a law abiding fermion, what a perfectly chilly day for keeping cooling Quantums…and who best to talk Quantum coolness than Deutsches Zentrum für Luft-und Raumfahrt (DLR)’s Quantum Queen #LisaWoerner! I cannot FREAKING wait to be talking with her again today on I’m With (Stargate) Genius…live,…if you’re cool enough, that is!

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A graduate research assistant at The University of Alabama in Huntsville (UAH), a part of The University of Alabama system, has published a paper in the journal Astronomy & Astrophysics that builds on an earlier study to help understand why the solar corona is so hot compared to the surface of the sun itself.

To shed further light on this age-old mystery, Syed Ayaz, a Ph.D. candidate in the UAH Center for Space Plasma and Aeronomic Research (CSPAR), employed a statistical model known as a Kappa distribution to describe the velocity of particles in space plasmas, while incorporating the interaction of suprathermal particles with kinetic Alfvén waves (KAWs).

KAWs are oscillations of the charged particles and as they move through the , caused by motions in the photosphere, the sun’s outer shell. The waves are a valuable tool for modeling various phenomena in the solar system, including particle acceleration and wave-particle interactions.

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Researchers have devised a method that bridges the gap between simulations and real-world dynamics, paving the way for faster innovation in energy-efficient computing.

Magnetic Whirls: The Future of Data Storage?

Skyrmions are tiny magnetic whirlpools, ranging from nanometers to micrometers in size, that behave like particles and can be easily controlled with electrical currents.

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Quantum field theory suggests that the very structure of the universe could change, altering cosmos as we know it. A new quantum machine might help probe this elusive phenomenon, while also helping improve quantum computers.

Nearly 50 years ago, quantum field theory researchers proposed that the universe exists in a “false vacuum”. This would mean that the stable appearance of the cosmos and its physical laws might be on the verge of collapse. The universe, according to this theory, could be transitioning to a “true vacuum” state.

The theory comes from predictions about the behaviour of the Higgs field associated with the Higgs boson, which Cosmos first looked at nearly a decade ago – the article is worth reading.

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