Scientists discover new phenomenon in chiral symmetry breaking
Peer-Reviewed Publication
Updates every hour. Last Updated: 28-Dec-2025 05:11 ET (28-Dec-2025 10:11 GMT/UTC)
Researchers at The University of Osaka have discovered a new type of chiral symmetry breaking (CSB) in an organic crystalline compound. This phenomenon, involving a solid-state structural transition from an achiral to a chiral crystal, represents a significant advance in our understanding of chirality and offers a simplified model to study the origin of homochirality. This transformation also activates circularly polarized luminescence, enabling new optical materials with tunable light properties.
A team of researchers has unveiled a powerful imaging technique that captures a full-dimensional portrait of elusive trap states—defects that hinder the performance of perovskite solar cells. By combining scanning photocurrent measurement system (SPMS) with complementary tools like thermal admittance spectroscopy (TAS) and drive-level capacitance profiling (DLCP), the team produced detailed spatial and energy maps of these hidden imperfections. Leveraging these insights, they introduced a passivation strategy using sulfa guanidine molecules that dramatically improved device performance. The result: a record-breaking solar cell achieving 25.74% efficiency. This breakthrough not only unlocks a deeper understanding of device physics but also provides a practical pathway to next-generation solar technologies.
Supernovae appear to our eyes—and to astronomical instruments—as brilliant flashes that flare up in the sky without warning, in places where nothing was visible just moments before. The flash is caused by the colossal explosion of a star. Because supernovae are sudden and unpredictable, they have long been difficult to study, but today, thanks to extensive, continuous, high-cadence sky surveys, astronomers can discover new ones almost daily.
It is crucial, however, to develop protocols and methods that detect them promptly; only in that way can we understand the events and celestial bodies that triggered them. In a pilot study, Lluís Galbany of the Institute of Space Sciences (ICE-CSIC) in Barcelona and his colleagues present a methodology that can obtain the earliest possible spectra of supernovae—ideally within 48 hours, or even 24 hours, of the “first light.” The results have just been published in the Journal of Cosmology and Astroparticle Physics (JCAP).
Biological tissues like skin, arteries, and cartilage have a non-linear strain-stiffening relationship. Some biomimetic hydrogel scaffolds have been successful in effectively replicating this behavior. However, achieving structural complexity in such strain-stiffening hydrogels has been difficult. A recent Research study has demonstrated an innovative and efficient technique, immersion phase separation 3D printing, to fabricate structurally complex tissues with strain-stiffening properties. These hydrogel scaffolds can pave the way for biomimetic, patient-specific implants in the future.
Researchers from The University of Osaka used electricity to drive a reaction to form a novel hetero[8]circulene consisting of five hexagons and three pentagons (called a dioxaza[8]circulene). The dioxaza[8]circulene is unsymmetrical, unlike existing hetero[8]circulenes. The novel molecule can be produced from commercially available materials by a two-step method that simultaneously forms six new bonds with only water as a byproduct. The dioxaza[8]circulene may have potential as a photocatalyst, and be used to speed up reactions triggered by light.