
A research team from the Institute of Modern Physics has directly measured the masses of two highly unstable atomic nuclei, phosphorus-26 and sulfur-27. These precise measurements provide crucial information for determining the nuclear reaction rate during X-ray bursts, advancing our understanding of how elements are synthesized under such extreme conditions.
A research team led by Prof. LIU Fanglin from the Hefei Institutes of Physical Science of the Chinese Academy of Sciences has developed a novel generative model-based method for ecological soundscape analysis.
A new study led by the Yunnan Observatories of the Chinese Academy of Sciences has detected quasi-periodic oscillation (QPO) signals in an unusual gamma-ray burst (GRB) event.
Using high-precision astrometry from the Gaia satellite and applying uniform, stringent selection criteria, researchers from the Xinjiang Astronomical Observatory have identified 400 candidate binary open clusters in the Milky Way; 268 of these were newly reported. The findings provide a unified, structured scheme for identifying and classifying galactic binary clusters.
A latest cosmological simulation study by researchers from the Shanghai Astronomical Observatory has systematically revealed, for the first time, how the interaction between dark matter and dark energy significantly influences the rotation and shape alignment of dark matter halos in the universe.
Researchers from the Hefei Institutes of Physical Science of the Chinese Academy of Sciences have developed advanced robotic technologies to support the assembly and maintenance of future fusion reactors, addressing the critical challenge of operating heavy robotic arms with extreme precision in complex and hazardous environments.
86-10-68597521 (day)
86-10-68597289 (night)
52 Sanlihe Rd., Xicheng District,
Beijing, China (100864)