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Subatomic Physics

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524 The Shell Model<br />

has an excitation energy that is nearly 2 MeV larger than that of the other isotopes.<br />

Figure 17.3: Ground and first-excited states of the even-A<br />

isotopes of Pb.<br />

17.2 The Closed Shells<br />

Furthermore, unlike all the<br />

other isotopes for which the<br />

spins and parities of the first<br />

excited states are 2 + ,thatof<br />

208 Pb is 3 − . The closed shell<br />

affects not only the energy of<br />

the first excited state but also<br />

its spin and parity.<br />

The first task in the construction of the shell model is the explanation of the magic<br />

numbers. In the independent-particle model it is assumed that the nucleons move<br />

independently in the nuclear potential. Because of the short range of the nuclear<br />

forces, this potential resembles the nuclear density distribution. To see the resemblance<br />

explicitly, we consider a two-body force of the type<br />

V12 = V0f(x1 − x2), (17.4)<br />

where V0 is the central depth of the potential and f describes its shape. The<br />

function f is assumed to be smooth and of very short range. A crude estimate<br />

of the strength of the central potential acting on nucleon 1 in the nucleus can be<br />

obtained by averaging over nucleon 2. Such an averaging represents the action of all<br />

nucleons (except 1) on 1. Averaging is performed by multiplying V12 by the density<br />

distribution of nucleon 2 in the nucleus, ρ(x2),<br />

�<br />

V (1) = V0 d 3 x2f(x1 − x2)ρ(x2).<br />

If f is of sufficiently short range, ρ(x2) can be approximated by ρ(x1), and V (1)<br />

becomes<br />

�<br />

V (1) = CV0ρ(x1), C = d 3 xf(x). (17.5)<br />

The potential seen by a particle is indeed proportional to the nuclear density distribution.<br />

The density distribution, in turn, is approximately the same as the charge<br />

distribution. The charge distribution of spherical nuclei was studied in Section 6.4,<br />

and it was found that it can be represented in a first approximation by the Fermi<br />

distribution, Fig. 6.4. It would therefore be appropriate to start the investigation<br />

of the single-particle levels by using a potential that has the form of a Fermi distribution<br />

but is attractive. The Schrödinger equation for such a potential cannot be

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