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Sporotrichosis, a neglected tropical disease caused by Sporothrix species, is a growing concern, particularly due to the emergence of highly virulent, cat-transmitted S. brasiliensis. Rapid diagnosis and surveillance are crucial for controlling sporotrichosis. This study investigated the 3-carboxymuconate cyclase (CMC) gene, which encodes the major Sporothrix antigen (Gp60–70), as a molecular marker to understand the genetic diversity and evolution of these fungi. Analysis of 104 isolates (S. brasiliensis, S. schenckii, S. globosa, and S. luriei) revealed 79 unique haplotypes, demonstrating superior discriminatory power over traditional molecular markers. High–CMC polymorphisms, especially in S. brasiliensis and S. schenckii, suggest recent population expansion or positive selection, potentially driven by environmental pressures such as polyaromatic hydrocarbon pollutants. The conserved chromosomal location of CMC in pathogenic Sporothrix and its absence in less virulent species suggest a role in virulence. Identifying conserved residues within predicted B-cell epitopes provides targets for diagnostics and therapeutics. Additionally, we identified N-linked glycosylation sequons (e.g. NGS at 62, NNT at 225, and NGT at 373/374) conserved in pathogenic Sporothrix but absent in environmental Sordariomycetes, possibly contributing to pathogenicity and niche adaptation. This study establishes CMC as a valuable marker for understanding Sporothrix evolution and virulence, aiding in sporotrichosis management.

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Researchers from the Henry and Marilyn Taub Faculty of Computer Science have developed an AI-based method that accelerates DNA-based data retrieval by three orders of magnitude while significantly improving accuracy. The research team included Ph.D. student Omer Sabary, Dr. Daniella Bar-Lev, Dr. Itai Orr, Prof. Eitan Yaakobi, and Prof. Tuvi Etzion.

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Company behind the Radian One experimental single stage to orbit spaceplane has announced its advanced Dur-E-Therm spacecraft material.

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The heating effect of microwaves has long been used to accelerate reactions. A new experiment shows that microwaves can also excite molecules into a less reactive state.

According to Arrhenius’ law, heating increases the energy of molecules so that more of them can overcome the activation barrier and undergo a chemical reaction. One way to deliver heat is via microwave radiation. Since its early use in chemical synthesis, scientists have noticed that microwave-induced reactions often proceed differently compared with ones enhanced with oil baths and other traditional heating methods. This finding has led to ongoing speculation and debate—and even controversy—about the existence of microwave effects beyond heating [1]. Now Valentina Zhelyazkova of the Swiss Federal Institute of Technology (ETH) Zurich and her collaborators have demonstrated that microwaves can both speed up and slow down chemical reactions [2]. The discovery provides clear evidence of the nonthermal influence of microwaves on chemical processes. It also opens a path toward controlling reactions and understanding them more deeply.

In their investigation Zhelyazkova and her collaborators manipulated the rate of the gas-phase reaction between positively charged helium ions (He+) and carbon monoxide (CO) molecules: He++ CO → He + C++ O. According to so-called capture theory, the reaction’s rate depends on the rotational states of CO, whose quantized energies lie within the microwave band (Fig. 1). The experiment began with the preparation of separate supersonic beams of He atoms and CO molecules via high-pressure expansion into vacuum. The CO molecules were initially in the rotational ground state. By applying a precisely timed microwave pulse before the reaction, the researchers excited a fraction of the population to the first rotationally excited state, which is less reactive than the ground state. The fraction that was excited could be fine-tuned by changing the duration of the microwave pulse.

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Researchers at TU Delft and Brown University have developed scalable nanotechnology-based lightsails that could support future advances in space exploration and experimental physics. Their research, published in Nature Communications, introduces new materials and production methods to create the thinnest large-scale reflectors ever made.

Lightsails are ultra-thin, reflective structures that use laser-driven radiation pressure to propel spacecraft at high speeds. Unlike conventional nanotechnology, which miniaturizes devices in all dimensions, lightsails follow a different approach. They are nanoscale in thickness—about 1/1000th the thickness of a human hair—but can extend to sheets with large dimensions.

Fabricating a as envisioned for the Breakthrough Starshot Initiative would traditionally take 15 years, mainly because it is covered in billions of nanoscale holes. Using advanced techniques, the team, including first author and Ph.D. student Lucas Norder, has reduced this process to a single day.

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Imagine building a Lego tower with perfectly aligned blocks. Each block represents an atom in a tiny crystal, known as a quantum dot. Just like bumping the tower can shift the blocks and change its structure, external forces can shift the atoms in a quantum dot, breaking its symmetry and affecting its properties.

Scientists have learned that they can intentionally cause symmetry breaking—or symmetry restoration—in quantum dots to create new materials with unique properties. In a recent study, researchers at the U.S. Department of Energy’s (DOE) Argonne National Laboratory have discovered how to use light to change the arrangement of atoms in these minuscule structures.

Quantum dots made of semiconductor materials, such as lead sulfide, are known for their unique optical and due to their tiny size, giving them the potential to revolutionize fields such as electronics and medical imaging. By harnessing the ability to control symmetry in these quantum dots, scientists can tailor the materials to have specific light and electricity-related properties. This research opens up new possibilities for designing materials that can perform tasks previously thought impossible, offering a pathway to innovative technologies.

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Using the Green Bank Telescope (GBT), astronomers have detected a new giant molecular cloud in the Milky Way galaxy. The newfound cloud has a size of nearly 200 light years and its mass is estimated to be some 160,000 solar masses. The finding was reported in a paper published March 18 on the arXiv preprint server.

Molecular clouds are huge complexes of interstellar gas and left over from the formation of galaxies, composed mostly of . Molecular clouds with masses greater than 100,000 solar masses are called (GMCs). In general, GMCs are 15–600 light years in diameter and are the coldest and densest parts of the interstellar medium.

GMCs are gas reservoirs where most takes place. Therefore, studying their lifecycle and characteristics is crucial to advancing our knowledge about the formation and evolution of galaxies.

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Does the proton decay? While this was a famous prediction of Grand Unified Theories (GUTS) developed in the 1970s and 1980s, experimentalists have ruled it out—or rather, put lower limits on its mean lifetime of about 1034 years. That’s 20 orders of magnitude greater than the age of the universe.

But two physicists have been wondering: Could the lifetime be different in other places and at other times? Could the proton have decayed faster in the past? Could it decay faster somewhere else in the universe? They have reimagined some physics processes assuming the proton does decay and calculated possible lifetimes of around 1018 years. That’s only eight orders of magnitude beyond the universe’s lifetime. Their work was recently published in Physical Review D.

“People had previously asked various questions of the type, ‘Are the fundamental physics parameters measured on the Earth the same elsewhere in the universe?’” said Peter Denton, a co-author at Brookhaven National Laboratory on Long Island, New York in the U.S. “One case that hadn’t been investigated was the stability of the proton. Earth experiments show that the proton is incredibly stable, but those only apply here, in our part of the galaxy, and now, over the last several decades. What if proton decay depended on time or space?”

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