Superheavy Elements: A Crossroads
@article{Seaborg1979SuperheavyEA, title={Superheavy Elements: A Crossroads}, author={Glenn Theodore Seaborg and W. Loveland and David J. Morrissey}, journal={Science}, year={1979}, volume={203}, pages={711 - 717} }
The failure to synthesize superheavy elements by using complete fusion reactions is most likely understandable in terms of the low survival probabilities of the superheavy precursors formed in these reactions or (in some cases) the failure to achieve complete fusion. Further attempts to synthesize these elements by using complete fusion or deep inelastic transfer reactions, or both, are discussed in light of these results.
31 Citations
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Microscopic nuclear theories predict a region of superheavy elements (SHEs) at the next doubly magic shell closure above 208Pb. Early models locate the shell closure at Z = 114,more recent…
Chemistry of superheavy elements.
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These results place the architecture of the far-end of the Periodic Table on the test bench and probe the increasingly strong relativistic effects that influence the chemical properties there.
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A test bench is established to challenge the validity and predictive power of modern fully relativistic quantum chemical models and to probe ‘relativistically’ influenced chemical properties and the architecture of the periodic table at its farthest reach.
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