Primordial Superheavy Element 126
- 13 September 1976
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 37 (11) , 664-666
- https://doi.org/10.1103/physrevlett.37.664
Abstract
Based on the shell corrections obtained from an extrapolated potential, the superheavy nucleus 126 in a spherical configuration does not appear to have a half-life as long as the age of the universe. Hartree-Fock calculations with Skyrme interactions do not reveal extra stability for element 126 (). There is thus the possibility that the primordial superheavy element 126 observed by Gentry et al may not be spherical. The distinction between spherical and toroidal shapes can be made by measuring the mass number of the observed superheavy element.
Keywords
This publication has 11 references indexed in Scilit:
- Evidence for Primordial Superheavy ElementsPhysical Review Letters, 1976
- Nuclear ground-state properties and self-consistent calculations with the skyrme interactionNuclear Physics A, 1975
- Hartree-Fock Calculations with Skyrme's Interaction. II. Axially Deformed NucleiPhysical Review C, 1973
- Calculation of half-lives for superheavy nucleiNuclear Physics A, 1972
- Hartree-Fock Calculations with Skyrme's Interaction. I. Spherical NucleiPhysical Review C, 1972
- Closed shells for very heavy nucleiNuclear Physics A, 1971
- On the nuclear structure and stability of heavy and superheavy elementsNuclear Physics A, 1969
- and () Reactions with 50-MeV DeuteronsPhysical Review B, 1969
- “Shells” in deformed nucleiNuclear Physics A, 1968
- Additional evidence of stability of the superheavy element 310126 according to the shell modelPhysics Letters, 1966