The Nuclear Shell Model

We see that the atomic shell model works even though the hydrogen states are not very good approximations due to the coulomb repulsion between electrons. It works because of the tight binding and simplicity of closed shells. This is based on angular momentum and the Pauli principle.

Even with the strong nuclear force, a shell model describes important features of nuclei. Nuclei have tightly bound closed shells for both protons and neutrons. Tightly bound nuclei correspond to the most abundant elements. What elements exist is governed by nuclear physics and we can get a good idea from a simple shell model. Nuclear magic numbers occur for neutron or proton number of 2, 8, 20, 28, 50, 82, and 126. Nuclei where the number of protons or neutrons is magic are more tightly bound and often more abundant. Heavier nuclei tend to have more neutrons than protons because of the coulomb repulsion of the protons (and the otherwise symmetric strong interactions). Nuclei which are doubly magic are very tightly bound compared to neighboring nuclei. $_{82}{\mathrm Pb}^{208}$ is a good example of a doubly magic nucleus with many more protons than neutrons.

Remember, its only hydrogen states which are labeled with a principle quantum number $n=n_r+\ell+1$. In the nuclear shell model, $n$ refers only to the radial excitation so states like the $1h_{9\over 2}$ show up in real nuclei and on the following chart. The other feature of note in the nuclear shell model is that the nuclear spin orbit interaction is strong and of the opposite sign to that in atoms. The splitting between states of different $j$ is smaller than but of the same order as splitting between radial or angular excitations. It is this effect and the shell model for which Maria Mayer got her Nobel prize.