2011
DOI: 10.1524/ract.2011.1860
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Synthesis of the heaviest elements in 48Ca-induced reactions

Abstract: Summary. 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.

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Cited by 137 publications
(68 citation statements)
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“…[1][2][3] Syntheses of SHE with proton number Z up to 118 have been reported. 4 Elements with Z=104-112 are members of the 6d series in the Periodic Table of the Elements. The 7p valence shell is expected to be filled in the elements with Z=113-118.…”
Section: Introductionmentioning
confidence: 99%
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“…[1][2][3] Syntheses of SHE with proton number Z up to 118 have been reported. 4 Elements with Z=104-112 are members of the 6d series in the Periodic Table of the Elements. The 7p valence shell is expected to be filled in the elements with Z=113-118.…”
Section: Introductionmentioning
confidence: 99%
“…The chromatography channel is made of silicon detectors for the detection of  particles and spontaneous fission (SF) fragments. This approach was successfully applied for the first time in chemical studies on HsO 4 . 17 Cn was investigated by thermochromatography on a Au surface.…”
Section: Introductionmentioning
confidence: 99%
“…Consequently, three to five neutrons are emitted before the compound nucleus has cooled. Still, because of the neutron-richness of actinides targets, these reactions yield the more neutron-rich, rela- tively long-lived isotopes used in chemical investigations of SHE; see Table 2 for used nuclides and [25,32,37,38,60,78,79] for more details.…”
Section: Nuclear Syntheses and Decaysmentioning
confidence: 99%
“…This isotope, as we know it today, predominantly shows α-decay with a half-life of 3.8 s and is produced with a cross section of about 2 pb [32,35] or less [34]. Even if the authors published the observation of Cn, today, we must conclude that these early experiments did not convincingly identify 283 Cn, mostly because of false assumptions about decay properties (T 1/2 = 3 min, SF) and assuming a too high cross section; all based on the knowledge of the early 2000s.…”
Section: Copernicium (Cn Element 112)mentioning
confidence: 99%
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