Portable field surveillance reveals how untreated sewage is reshaping coastal microbial communities and spreading diverse resistance genes across one of the world’s most protected marine environments.
If scientists could find a material that acts as a superconductor—that is, one that transmits energy with zero resistance—at normal pressures and relatively high temperatures, it would open up a vast number of possibilities. These include medical imaging, quantum computing and numerous other fields. So, yes, it would be a big deal.
“Right now, almost 50% of the energy in transmission is just heat in copper wires,” said Shomeek Mukhopadhyay. “If you can transmit electricity through wires without dissipating energy, that’s a huge economic benefit. I would say it’s equivalent to having thermonuclear fusion.”
Mukhopadhyay, a research scientist in Chemical & Environmental Engineering, is on the third floor of the Kline Geology Laboratory. Nearby, Natalia Nevskaya, a postdoctoral associate in Earth & Planetary Sciences, prepares a massive device called the Kawai multi-anvil press.
When humans and other animals move through familiar or unfamiliar environments, their brains rely on numerous intricate neural processes to decide which path to take next. Past studies have identified a specific population of cells in the hippocampus, a structure deep within the brain, that appears to play a key role in spatial navigation.
These cells, called place cells, become active when an animal either visits or thinks about a specific location. Place cells often fire in rapid sequences during so-called theta oscillations (i.e., rhythmic brain activity patterns that cycle approximately 4–12 times per second). These rapid bursts of sequential place cell activity, also known as theta sweeps, were previously associated with the mental evaluation of possible future routes.
Two distinct research teams based at Cornell University and University College London recently shed new light on the contribution of theta sweeps to spatial navigation.
A new study analyzing the James Webb Space Telescope (JWST) spectra of more than 1,400 galaxies suggests a surprisingly small group of “leaky” galaxies was responsible for cosmic reionization. The paper outlining this work was posted to the arXiv preprint server on July 24.
Cosmic reionization happened when ionizing ultraviolet radiation from early stars and galaxies heated the universe’s neutral hydrogen gas and converted it into the ionized state seen today. Based on cosmic microwave background and quasar data, this epoch is estimated to have occurred around redshift 6–8, roughly 600 million to 1 billion years after the Big Bang. The main driver is thought to be star-forming galaxies. Therefore, the epoch of reionization is considered the last major phase transition of the universe.
The ultraviolet radiation responsible for cosmic reionization is mainly composed of Lyman continuum (LyC) photons with wavelengths less than 912 Å. Their escape fraction from galaxies, along with the rate of their production, determines whether they reach and ionize the intergalactic medium because most LyC photons are absorbed internally by gas and dust.
Today’s quantum technologies rely on energy-intensive lasers, raising concerns that scaling them up could further increase energy demands. In new work, researchers have demonstrated that quantum entanglement between photons can be generated directly from sunlight, offering a potential alternative.
“Quantum entanglement is crucial for applications such as secure communication, ultra-precise sensing and high-performance computation,” said Cheng Li, a recent graduate of the University of Ottawa in Canada. “Our work shows that abundant natural light sources can be used for quantum entanglement, opening the possibility of more energy-efficient and accessible quantum technologies.”
In Optica, the researchers report that the entanglement they achieved using sunlight was comparable to laser-based approaches after accounting for differences in the bandwidth of the input light.
Quantum errors are a normal part of quantum computing because fragile physical qubits (the tiny components storing data) can easily break down because of environmental noise, like heat, stray signals or microscopic vibrations. Typical fixes involve vast amounts of extra hardware qubits, which make computers larger, more expensive and harder to build.
In a paper published in the journal Nature, scientists report developing a two-qubit entangling gate that automatically flags its most common errors as they occur.
The team at D-Wave Quantum Inc. engineered an ultrafast link, called a controlled-Z (CZ) entangling gate, that entangles two qubits in just 500 nanoseconds. When errors occur, the system automatically flags most of them as photon losses (known as erasures) instead of letting them turn into hidden glitches.
Narrow jets of luminous matter may be emitted toward Earth from the nuclei of active galaxies billions of light-years away. The galaxy then appears as a point source and is called a blazar. A Polish-German team of scientists has, for the first time, analyzed the activity of one such blazar over an extended period and, instead of finding answers, encountered an ever-increasing number of intriguing questions.
Distant, active galaxies that emit jets of matter at small angles toward Earth, known as blazars, present astronomers with numerous observational and interpretative challenges. Their immense distance and specific orientation, combined with the high variability of the emitted radiation—which, moreover, is generated across a very wide energy range—are the main reasons why understanding the phenomena responsible for the properties of blazars is particularly difficult.
Are the current interpretations of the nature of these objects, based on short-term and rather sporadic observations, correct? A group of scientists from the University of Heidelberg and the Institute of Nuclear Physics of the Polish Academy of Sciences (IFJ PAN) in Krakow set out to answer this question. The research carried out on the Polish side focused on the blazar PKS 2155-304, located one and a half billion light-years away. It is situated in the southern celestial hemisphere, in the background of the constellation Piscis Austrinus. The paper is published in the Journal of High Energy Astrophysics.
Fluorescent dyes have long been used in biological research to identify and visualize structures within living cells. Although effective, they have several drawbacks, including altering the cells under study, limiting the number of structures that can be examined at once and reducing measurement accuracy.
A team led by University at Buffalo researchers has developed a new method that draws on advances in artificial intelligence and Raman spectroscopy to overcome the limitations of dye-based imaging.
The approach combines AI with “Ramanomics,” a UB-pioneered optical technology that measures the biochemical makeup of cells without altering them. Rather than relying on fluorescent labels, which are dyes that bind to specific cellular components and glow under specialized lighting, it identifies cellular structures by their unique biochemical signatures.