Could cardamom seeds be a potential source of antiviral treatment?
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Updates every hour. Last Updated: 26-Dec-2025 18:11 ET (26-Dec-2025 23:11 GMT/UTC)
Hydrogen is a promising fuel for developing sustainable industrial processes, but its use is hindered by hydrogen embrittlement—a phenomenon that weakens metals and can cause sudden failure. Now, researchers from Japan have provided the first experimental evidence linking surface roughness to atomic-scale defects caused by hydrogen in iron. Using positron annihilation lifetime spectroscopy, they showed that rougher surfaces result in greater accumulation of defects, offering new insights into designing hydrogen-resistant materials through precision surface engineering.
A deep blue organic light-emitting diode (OLED) developed by researchers at Science Tokyo operates on just a single 1.5 V, overcoming the high-voltage and color-purity problems that have long limited blue OLEDs. The breakthrough was achieved by introducing a new molecular dopant that prevents charge trapping, a problem that previously hampered the performance of low-voltage OLEDs. The resulting device produces sharp blue emission that meets BT.2020 standards, paving the way toward brighter, more energy-efficient displays.
Sodium-ion batteries (SIBs) are a promising, low-cost alternative to lithium-ion batteries for both personal electronics and large-scale energy storage, but their adoption is limited by their poor stability in air and water. In a recent study, researchers from Japan addressed this challenge by doping the SIB cathode material Na2/3[Fe1/2Mn1/2]O2 with calcium. This simple modification greatly improved stability and performance, paving the way for more practical and sustainable battery technologies.
The University of Osaka scientists have developed a safe, efficient “dump-and-stir” method to introduce ortho-carborane into various aromatic compounds using a newly designed lithium–copper reagent. This innovation overcomes the complexity and hazards of previous methods, paving the way for new applications in boron neutron capture therapy (BNCT), three-dimensional aromatic materials, and bioisosteric drug design.
Kyoto, Japan -- White dwarfs are the compact remnants of stars that have stopped nuclear burning, a fate that will eventually befall our sun. These extremely dense objects are degenerate stars because their structure is counterintuitive: the heavier they are, the smaller they are.
White dwarfs often form binary systems, in which two stars orbit one another. The majority of these are ancient even by galactic standards, and have cooled to surface temperatures of about 4,000 degrees Kelvin. However, recent studies have revealed a class of short period binary systems in which the stars orbit each other faster than once per hour. Contrary to theoretical models, these stars are inflated to twice the size as expected due to surface temperatures of 10 to 30 thousand degrees Kelvin.
This inspired a team of researchers, led by Lucy Olivia McNeill of Kyoto University, to investigate the theory of tides and use it to predict the temperature increase of white dwarfs in short period binary orbits. Tidal forces often deform celestial bodies in binary orbits, determining their orbital evolution.