Why should elements beyond, say, atomic number exist at all? One might think that the Coulomb repulsion of so many protons ought to make such nuclei fission. But elements with a Z as high as 112 have been created, and they prefer to decay by alpha emission instead of fission. So it's widely believed that the relative stability of these high‐Z nuclei is a striking example of nuclear shell structure, which lowers the energy of the ground state, thereby creating a fission barrier. Without the shell‐correction energy, the heaviest nuclei wouldn't be stable.
This content is only available via PDF.
© 1999 American Institute of Physics.
1999
American Institute of Physics
You do not currently have access to this content.