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Subatomic Physics

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17.5. Generalization of the Single-Particle Model 533<br />

The foreign states are not really foreign. While they cannot be described in terms<br />

of the extreme single-particle shell model, they can be understood in terms of the<br />

general shell model, through excitations from the core. In the case of 209 Pb, the<br />

first such state appears at 2.15 MeV. The estimate based on Figs. 17.2 and 17.3<br />

that core excitation will play a role at about 2 MeV is verified.<br />

Figure 17.11: Excited states in 57 Ni and 209 Pb. The states<br />

that allow an unambiguous shell-model assignment are labeled<br />

with the corresponding quantum numbers.<br />

We have discussed only two<br />

properties of nuclei that are<br />

well described by the singleparticle<br />

model, spin and parity<br />

of ground states and the<br />

level sequence and quantum<br />

numbers of the lowest excited<br />

states. There are other<br />

features that are explained<br />

by the extreme single-particle<br />

model, for instance the existence<br />

of very-long-lived first<br />

excited states in certain regions<br />

of N and Z, the socalled<br />

islands of isomerism.<br />

However, the model applies only to a restricted class of nuclei—namely those with<br />

only one nucleon outside a closed shell—and an extension to more general conditions<br />

is necessary.<br />

17.5 Generalization of the Single-Particle Model<br />

The extreme single-particle shell model, discussed in the previous section, is based<br />

on a number of rather unrealistic assumptions: The nucleons move in a spherical<br />

fixed potential, no interactions among the particles are taken into account, and<br />

only the last odd particle contributes to the level properties. These restrictions are<br />

removed in various steps and to various degrees of sophistication; we briefly outline<br />

some of the extensions.<br />

1. All particles outside the closed major shells are considered. The angular momenta<br />

of these particles can be combined in various ways to get the resulting<br />

angular momentum. The two main schemes are the Russell–Saunders, or LS,<br />

coupling, and the jj coupling. In the first, the orbital angular momenta are<br />

assumed to be weakly coupled to the spins; spin and orbital angular momenta<br />

of all nucleons in a shell are added separately to get the resulting L and

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