Shell evolution and its indication on the isospin dependence of the spin-orbit splitting

preprint2013arXivOpen access

Abstract

The available experimental data on shell evolution indicate that the strength of the spin-orbit (SO) single-particle potential may be enhanced in neutron-rich nuclei. We observe that such a simple scheme destroys the Harmonic Oscillator (HO) magic numbers N=8 and 20 and generates new SO magic numbers like N=6, 14, 16, 32 and 34. The traditional SO magic numbers like N=28 and 50 and N=14 seen in 22^{22}O are eroded somehow in neutron-rich nuclei due to the sensitivity of larger-ll orbitals to the depth of the central potential but they are more robust than the HO magic numbers. The N=82 shell closure persists in neutron-rich nuclei while HO shell closures like N=40 and 70 do not emerge. Both mechanisms contribute to enhancing the N=56 and 90 gaps by splitting the 1d5/21d_{5/2} and 0g7/20g_{7/2} and the 0h9/20h_{9/2} and 1f7/21f_{7/2} orbitals.

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