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• W2002912157 startingPage "082003" @default.
• W2002912157 abstract "The observation of atomic numbers Z by 40% larger than that of Bi, the heaviest stable element, is an impressive extension in 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 SHN to exist. The fundamentals of the modern theory concerning the mass limits of nuclear matter have thus obtained experimental verification." @default.
• W2002912157 created "2016-06-24" @default.
• W2002912157 creator A5018135472 @default.
• W2002912157 date "2011-09-23" @default.
• W2002912157 modified "2023-09-25" @default.
• W2002912157 title "Heaviest Nuclei from48Ca-induced Reactions" @default.
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• W2002912157 doi "https://doi.org/10.1088/1742-6596/312/8/082003" @default.
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