Lifeboat Foundation

Research laboratories are constantly developing new materials that are expected to exhibit novel properties bound to revolutionize this or that technology. But it’s not enough to simply create these materials; scientists also need to find efficient methods of processing and fine-tuning them.

Moreover, composites are often made via the addition of nanoparticles into a base matrix, which is why it is necessary to find a way of manipulating the location, size, and concentration rate of these particles that would exclude even the smallest deviations that are invisible to the human eye.

Researchers from ITMO University have improved on the technique of local processing of composites based on nanoporous glass with addition of silver and copper. Now, it is possible to predict with high accuracy the optical properties of a plasmonic component during its treatment.

Professors from the Skoltech Center for Energy Science and Technology (CEST), Lomonosov Moscow State University and College de France shared their vision on the importance of solid state chemistry in advancements currently awaited from contemporary and prospective metal-ion batteries. The opinion was contributed as an invited review to Nature Communications.

Metal-ion batteries are the main drivers enabling a smooth transfer to renewables and green energy for a sustainable planet. The artfully designed electrode materials have greatly contributed to the development of high-performance Li-ion batteries that was eventually hallmarked by the 2019 Nobel Prize, which had signified the role solid state chemistry. Targeted design of novel metal-ion battery materials to bring the technology to the next level clearly stands as a great challenge for today’s chemistry community.

The individual properties of atoms and ions encoded in the Periodic Table along with the fundamental trends and principles multiplied by further levels of complexity constitute multitude of possible combinations for scientists to find new battery electrodes. Obviously, the researchers need solid guidelines while searching through this huge parameter space for the best chemical combinations and structures.

What happens if you turn space-time upside-down?

A cycle of false tabloid claims that NASA had discovered a “parallel universe” papered over a far deeper story about particles, the cosmos, and what happens when you turn spacetime upside-down.

Strangelets, and specifically nuclearites, their heavy species, are very dense, compact and potentially fast objects made of large and roughly equal numbers of up, down and strange quarks, which may inhabit the universe. Their existence was first hypothesized by Edward Witten back in 1984. These objects have never been detected before and have so far attracted less attention than meteors, perhaps due to their lack of relevance in particle physics.

At the end of 1984, theoretical physicists Alvaro De Rujula and Sheldon Lee Glashow introduced the idea that, when crossing the Earth’s atmosphere, nuclearites produce light in a similar way to meteors, losing very little of their energy in the process. If their prediction is right, teams working at meteor observatories should be able to confirm whether these objects exist or not. So far, however, very few researchers have conducted studies investigating this possibility.

A different cosmic phenomenon rooted in particle physics, known as ultra-high energy cosmic rayssome of the same theorized characteristics of nuclearites. These cosmic rays, in fact, also produce trails of light in the atmosphere, although they do this via a different physical process. In addition, they move much faster than nuclearities and are usually observed in the ultraviolet (UV) band.

So next week, as U.S. particle physicists start to drum up new ideas for the next decade in a yearlong Snowmass process—named for the Colorado ski resort where such planning exercises once took place—they have no single big project to push for (or against). And in some subfields, the next steps seem far less obvious than they were 10 years ago. “We have to be much more open minded about what particle physics and fundamental physics are,” says Young-Kee Kim of the University of Chicago and chair of the American Physical Society’s division of particles and fields, which is sponsoring the planning exercise.

Giant neutrino experiment is the only sure thing for the field.

A team of University of Arkansas physicists has successfully developed a circuit capable of capturing graphene’s thermal motion and converting it into an electrical current.

“An energy-harvesting circuit based on graphene could be incorporated into a chip to provide clean, limitless, low-voltage power for small devices or sensors,” said Paul Thibado, professor of physics and lead researcher in the discovery.

Continue reading “Physicists build circuit that generates clean, limitless power from graphene” »

Scientists have created a device which could make it easier to harness super-fast quantum computers for real-world applications, a team at Finland’s Aalto University said on Wednesday.

Quantum computers are a new generation of machines powered by energy transfers between so-called “artificial atoms”—electrical circuits a fraction of a millimetre across.

Scientists believe the devices will eventually be able to vastly outperform even the world’s most powerful conventional supercomputers.

Three United States DOE national laboratories – SLAC, Fermilab and Jefferson Lab – have partnered to build an advanced particle accelerator that will power the LCLS-II X-ray laser. Thanks to technology developed for nuclear and high-energy physics, the new X-ray laser will produce a nearly continuous wave of electrons and allow scientists to peer more deeply than ever before into the building blocks of life and matter.

Comet 67P/C-G is a dusty object. As it neared its closest approach to the Sun in late July and August 2015, instruments on Rosetta recorded a huge amount of dust enshrouding the comet.

This is tied to the comet’s proximity to our parent star, its heat causing the comet’s nucleus to release gases into space, lifting the dust along. Spectacular jets were also observed, blasting more dust away from the comet. This disturbed, ejected material forms the ‘coma’, the gaseous envelope encasing the comet’s nucleus, and can create a beautiful and distinctive tail.

A single image from Rosetta’s OSIRIS instrument can contain hundreds of dust particles and grains surrounding the 4 km-wide comet nucleus. Sometimes, even larger chunks of material left the surface of 67P/C-G — as shown here.