University of British Columbia (UBC) physicists may have solved one of nature’s great puzzles: what causes the accelerating expansion of our universe?

PhD student Qingdi Wang has tackled this question in a new study that tries to resolve a major incompatibility issue between two of the most successful theories that explain how our universe works: quantum mechanics and Einstein’s theory of general relativity.

Nanoengineers at the University of California San Diego have developed the first printed battery that is flexible, stretchable and rechargeable. The zinc batteries could be used to power everything from wearable sensors to solar cells and other kinds of electronics. The work appears in the April 19, 2017 issue of Advanced Energy Materials.  

The researchers made the printed batteries flexible and stretchable by incorporating a hyper-elastic polymer material made from isoprene, one of the main ingredients in rubber, and polystyrene, a resin-like component. The substance, known as SIS, allows the batteries to stretch to twice their size, in any direction, without suffering damage.

A new type of nanocatalyst can result in the long-awaited commercial breakthrough for fuel cell cars. Research results from Chalmers University of Technology and Technical University of Denmark show that it is possible to significantly reduce the need for platinum, a precious and rare metal, by creating a nanoalloy using a new production technique. The technology is also well suited for mass production.

“A nano solution is needed to mass-produce resource-efficient catalysts for fuel cells. With our method, only one tenth as much platinum is needed for the most demanding reactions. This can reduce the amount of platinum required for a fuel cell by about 70 per cent”, says Björn Wickman, researcher at the Department of Physics at Chalmers.

How can we burn natural gas without releasing CO2 into the air? This feat is achieved using a special combustion method that TU Wien has been researching for years: chemical looping combustion (CLC). In this process, CO2 can be isolated during combustion without having to use any additional energy, which means it can then go on to be stored. This prevents it from being released into the atmosphere.
The method had already been applied successfully in a test facility with 100 kW fuel power. An international research project has now managed to increase the scale of the technology significantly, thus creating all the necessary conditions to enable a fully functional demonstration facility to be built in the 10 MW range.

 

The spectacular variety of colours and patterns that butterflies use to ward off potential predators may result from highly localised environmental conditions known as “microhabitats”, researchers have found.

Nanometric-sized water drops are everywhere - in the air as droplets or aerosols, in our bodies as medication, and in the earth, within rocks and oil fields. To understand the behavior of these drops, it is necessary to know how they interact with their hydrophobic environment. This interaction takes places at the curved droplet interface, a sub-nanometric region that surrounds the small pocket of water. Researchers from EPFL, in collaboration with the institute AMOLF in the Netherlands, were able to observe what was going on in this particular region. They discovered that molecules on the surface of the drops were much more ordered than expected. Their surprising results have been published in Nature Communications. They pave the way to a better understanding of atmospheric, biological and geological processes.

“I’m strong to the finich, ‘cause I eats me spinach!” said Popeye the Sailor Man.

While you may not gulp spinach by the can-fuls, if you love spanakopita or your go-to appetizer is spinach artichoke dip, then you’ll be excited to know that new research out of Boyce Thompson Institute (BTI) will make it even easier to improve this nutritious and delicious, leafy green.

Pointing the National Science Foundation’s Very Large Array (VLA) at a famous galaxy for the first time in two decades, a team of astronomers got a big surprise, finding that a bright new object had appeared near the galaxy’s core. The object, the scientists concluded, is either a very rare type of supernova explosion or, more likely, an outburst from a second supermassive black hole closely orbiting the galaxy’s primary, central supermassive black hole.

When scientists develop the chemical formulas for new products such as fuels and medications, they often must first create molecules that haven’t previously existed.

A basic step toward creating new molecules is selectively breaking and re-forming the chemical bonds that connect the atoms that make them up. One of the chief challenges is that the bond between carbon and hydrogen atoms — the building blocks of many molecules — is exceptionally strong, so chemists often have to resort to using rare and expensive chemicals like iridium to convert it into other, more useful types of chemical bonds. Scientists refer to this process as “functionalizing” the bonds.

Axions are particles whose hypothetical existence was introduced in 1977 by Roberto Peccei and Helen Quinn. The particles have been the talk of the town lately because their existence could largely explain so-called dark matter. In order to make a solid claim, researchers have been measuring the interaction between axions and photons. A team of international scientists from the project CERN Axion Solar Telescope (CAST) at the European research center CERN in Geneva, Switzerland, including Prof. Dr. Horst Fischer from the Institute of Physics at the University of Freiburg, have set strict limits to the probability that axions turn into photons. They have presented their findings in the latest issue of Nature Physics.