Shell structure in neutron-rich Ca and Ni nuclei under semi-realistic mean fields
arXiv:1003.5720 · doi:10.1103/PhysRevC.81.051302
Abstract
Shell structure in the neutron-rich Ca and Ni nuclei is investigated by the spherical Hartree-Fock calculations with the semi-realistic interactions. Specific ingredients of the effective interaction, particularly the tensor force, often play a key role in the dependence of the neutron shell structure. Such examples are found in N=32 and N=40; N=32 becomes magic or submagic in Ca while its magicity is broken in Ni, and N=40 is submagic (though not magic) in Ni but not in Ca. Comments are given on the doubly magic nature of Ni. We point out that the loose binding can lead to a submagic number N=58 in Ni, assisted by the weak pair coupling.
14 pages including 5 figures, to appear in Physical Review C (Rapid Communication)
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- Emergence of new magic numbers N = 16 and 34 through tensor interaction in Skyrme Hartree Fock theory
- Can realistic interaction be useful for nuclear mean-field approaches?
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