Assessing competing fundamental magnetic interactions. From: Long-range ferrimagnetic order in a two-dimensional supramolecular Kondo lattice

Achieving magnetic order in low-dimensional systems consisting of only 1 or 2 dimensions has been a research goal for some time. In a new study published in the journal Nature Communications, Uppsala researchers show that magnetic order can be created in a two-dimensional chessboard lattice consisting of organometallic molecules that are only one atomic layer thick.

Magnetic order is a common phenomenon in 3D materials, such as ferromagnetic order in iron bar magnets, where the magnetic moments on all iron atoms point in the same direction...

a) Synthetic scheme of MoNi4 electrocatalyst supported by the MoO2 cuboids on nickel foam; b) polarization curves of the MoNi4 electrocatalyst supported by the MoO2 cuboids, pure Ni nanosheets and MoO2 cuboids on the nickel foam; c) calculated adsorption free energy diagram for the Tafel step.
Credit: Image courtesy of Technische Universitaet Dresden

A new paper from cfaed’s Chair for Molecular Functional Materials describes a new approach to revolutionize the production of molecular hydrogen. In many of the approaches for hydrogen production, the electrocatalytic hydrogen evolution reaction (HER) from water splitting is the most economical and effective route for the future hydrogen economy...

A visualization of a supercomputer simulation of merging black holes sending out gravitational waves. Credit: NASA/C. Henze Read more at: https://phys.org/news/2017-05-uncover-gravitational-characteristics.html#jCp

Monash researchers have identified a new concept – ‘orphan memory’ – which changes the current thinking around gravitational waves. Einstein’s theory of general relativity predicts that cataclysmic cosmic explosions stretch the fabric of spacetime. The stretching of spacetime is called ‘gravitational waves.’ After such an event, spacetime does not return to its original state. It stays stretched out. This effect is called ‘memory.’ The term ‘orphan’ alludes to the fact that the parent wave is not directly detectable.

“These waves could open the way for studying physics currently...

A false-color image map of the gas density in the Musca star-forming filament (the highest densities are shown in red). New theoretical work on the structure of these long filaments proposes several kinds of star-forming zones along the length and successfully reproduces many of the features seen in filaments like this one in Musca. Kainulainen, 2016

Interstellar molecular clouds are often seen to be elongated and “filamentary” in shape, and come in a wide range of sizes. In molecular clouds, where stars form, the filamentary structure is thought to play an important role in star formation as the matter collapses to form protostars...