Lifeboat Foundation

According to a new study of rivers and lakes in Wisconsin, natural foams from these bodies of water contain much higher concentrations of per-and polyfluoroalkyl substances (PFAS) than the water below them.

Thirty-six different kinds of PFAS compounds were analyzed in samples of both the foams and water surface microlayers of 43 Wisconsin rivers and lakes. The study, which is published in Environmental Science & Technology, also revealed that foams, generally off-white and found along shorelines, are not necessarily an indicator of elevated contamination levels in the entire water body.

“We studied many different lakes and found PFAS in all of them. The PFAS concentrations were high in the foams even if the concentrations in the water were relatively low,” said Christy Remucal, a professor with the University of Wisconsin–Madison Department of Civil and Environmental Engineering and interim director of the University of Wisconsin Aquatic Sciences Center.

For decades now, scientists have argued about how the universe is shaped, in the sense of complex parameters that govern the rules of space and time. Is it a simple open expanse, like a bigger version of the spaces we’re used to? Does it wrap around on itself like a donut? Or something even stranger?

Now, new research published in the journal Physical Review Letters, in the inaugural paper from a new consortium of cosmologists known as the COMPACT Collaboration, found that the “topology” of the universe — the shape of its geometry, basically — is likely anything but simple.

The researchers looked at the universe’s cosmic microwave background, which is basically the inherent “glow” of space, dating back to ancient radiation at the dawn of time.

Researchers have significantly improved gene-editing techniques. This new method, called eePASSIGE, can insert or replace entire genes in human cells with much higher efficiency than previous methods. This advancement could lead to a single gene therapy for diseases caused by various mutations in a single gene, like cystic fibrosis. Traditionally, gene therapy required a different treatment for each mutation.

EePASSIGE combines prime editing, which edits small stretches of DNA, with new enzymes that insert large pieces of DNA. This allows scientists to introduce a healthy copy of a gene directly where it belongs in the genome.

“This is one of the first examples of targeted gene integration with potential for therapeutic applications,” said Dr. David Liu, senior author of the study. “If these efficiencies translate to patients, many genetic diseases could be treated.”

Microbes that are used for health, agricultural, or other applications need to be able to withstand extreme conditions, and ideally the manufacturing processes used to make tablets for long-term storage. MIT researchers have now developed a new way to make microbes hardy enough to withstand these extreme conditions.

Their method involves mixing bacteria with food and drug additives from a list of compounds that the FDA classifies as “generally regarded as safe.” The researchers identified formulations that help to stabilize several different types of microbes, including yeast and bacteria, and they showed that these formulations could withstand high temperatures, radiation, and industrial processing that can damage unprotected microbes.

When atomic nuclei and subatomic particles interact, the results are incredibly complex. These are the “many body problems” of quantum mechanics. To help make sense of these interactions, scientists create ways to simplify the range of possible outcomes.

One example is “effective interactions,” which simplify the interactions between a nucleon (a proton or a neutron) and an atomic nucleus. Effective interactions help scientists develop theories of the reactions that result when nuclei collide with each other or with subatomic particles.

These tools are part of a group of methods called effective field theory (EFT). EFT in turn is a type of approach called “ab initio,” or “first principles.” Ab initio means a calculation starts with the established laws of physics without any other assumptions.

The findings could aid the hunt for these monstrous duos using gravitational waves, tiny ripples in space and time (united as a 4-dimensional entity called space-time), which were first predicted in Einstein’s theory of general relativity in 1915.

“These findings are useful for targeted searches for supermassive black hole binaries, in which we search specific galaxies and quasars for continuous gravitational waves from individual supermassive black hole binaries,” research lead author Andrew Casey-Clyde, a doctoral candidate at the University of Connecticut and visiting researcher at Yale University, told Space.com.

“Our results mean that these targeted searches will be up to seven times more likely to find gravitational waves from a supermassive black hole binary in a quasar than in a random massive galaxy,” Casey-Clyde said.

Researchers have developed a novel method for generating structured terahertz light beams using programmable spintronic emitters. This breakthrough offers a significant leap forward in terahertz technology, enabling the generation and manipulation of light with both spin and orbital angular momentum at these frequencies for the first time.

Terahertz radiation lies between microwaves and infrared light on the electromagnetic spectrum. It holds great promise for various applications, including security scanners, medical imaging, and ultrafast communication. However, generating and controlling terahertz light effectively has proven challenging.

This new research, published in eLight and led by Prof. Zhensheng Tao, Prof. Yizheng Wu from Fudan University and Prof. Yan Zhang from Capital Normal University, overcomes these limitations by employing programmable spintronic emitters based on exchange-biased magnetic multilayers. These devices consist of thin layers of magnetic and non-magnetic materials that convert laser-induced spin-polarized currents into broadband terahertz radiation.

Using the CARMENES spectrograph, astronomers have found evidence of water vapor in the atmosphere of a hot Saturn exoplanet designated HD 149,026 b, dubbed Smertrios. The finding, reported in a research paper published on the preprint server arXiv, could be key to a better understanding of the structure and formation scenario of this alien world.

Smertrios is a metal-rich hot Saturn orbiting HD 149026—a yellow subgiant star of spectral type G0 IV, at a distance of some 248.5 light years. The planet has a radius of about 0.81 Jupiter radii and is approximately three times less massive than Jupiter. Previous observations have found that Smertrios orbits its host every 2.876 days, about 0.043 AU from it. The planet’s equilibrium temperature is estimated to be 1,693 K.

The team of astronomers led by Sayyed A. Rafi of the University of Tokyo in Japan employed CARMENES at the Calar-Alto Observatory to conduct high-resolution cross-correlation spectroscopy of Smertrios. Their main aim was to get more insights into the composition of this exoplanet’s atmosphere.

Around 80% of the universe’s matter is dark, meaning it is invisible. Despite being imperceptible, dark matter constantly streams through us at a rate of trillions of particles per second. We know it exists due to its gravitational effects, yet direct detection has remained elusive.

Researchers from Lancaster University, the University of Oxford, and Royal Holloway, University of London, are leveraging cutting-edge quantum technologies to build the most sensitive dark matter detectors to date. Their project, titled “A Quantum View of the Invisible Universe,” is featured at the Royal Society’s Summer Science Exhibition. Related research is also published in the Journal of Low Temperature Physics

The team includes Dr. Michael Thompson, Professor Edward Laird, Dr. Dmitry Zmeev, and Dr. Samuli Autti from Lancaster, Professor Jocelyn Monroe from Oxford, and Professor Andrew Casey from RHUL.