2012/02/08 by Yu. Ts. Oganessian · 4 citations
Physics and Astronomy · #Nuclear physics research studies #Astronomical and nuclear sciences #Quantum Chromodynamics and Particle Interactions
paper · pdf · doi:10.1088/1742-6596/337/1/012005
openalex publication_date 2012/02/08 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/30
The observation of atomic numbers Z that are 40% larger than that of Bi, the heaviest stable element, is an impressive extension of nuclear survival. Although the super heavy nuclei (SHN) are at the limits of Coulomb stability, shell stabilization lowers the ground-state energy, creates a fission barrier, and thereby enables the SHE to exist. The fundamentals of the modern theory concerning the mass limits of nuclear matter have been experimentally verified.