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Subatomic Physics

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6.6. Nucleon Elastic Form Factors 153<br />

Figure 6.9: Strong and weak correction terms that appear in the interaction of a charged lepton<br />

with photons.<br />

quantum electrodynamics predicts all observed phenomena correctly if proper theoretical<br />

corrections, such as the strong vacuum polarization shown in Fig. 6.9, are<br />

carried out. Measurements in colliding beam experiments, in particular,<br />

e − e + −→ e − e + , e − e + −→ µ − µ + , and e − e + −→ τ − τ +<br />

show that QED holds to distances smaller than about 10 −18 m. (28) We consequently<br />

cannot yet answer the question raised by the incredible success of QED: Will the<br />

theory break down, and if so, at what scale?<br />

6.6 Nucleon Elastic Form Factors<br />

By 1932 it was well known that electrons have spin 1<br />

2 and a magnetic moment of<br />

1µB, (Bohr magneton), as predicted by the Dirac equation. Two other spin- 1<br />

2 particles<br />

were also known to exist, the proton and the neutron. It was firmly believed<br />

that these would also have magnetic moments as predicted by the Dirac equation,<br />

one nuclear magneton for the proton and zero moment for the neutron. Enter Otto<br />

Stern. Stern had principles in selecting his experiments: “Try only crucial experiments.<br />

Crucial experiments are those that test universally accepted principles.”<br />

When he started setting up equipment to measure the magnetic moment of the<br />

proton, his friends teased him and told him that he should not waste his time on an<br />

experiment whose outcome was foreordained. The surprise was great when Stern<br />

and his collaborators found a magnetic moment of about 2.5 µN for the proton and<br />

about −2 µN for the neutron. (29)<br />

How can the departure of the magnetic moments of the proton and the neutron<br />

from the “Dirac values” be understood? Before quarks were introduced, the explanation<br />

of the anomalous magnetic moments of the nucleons was based on virtual<br />

28K.G. Gan and M.L. Perl, Int. J. Mod. Phys. A3, 531 (1988).<br />

29I. Estermann, R. Frisch, and O. Stern, Nature 132, 169 (1933); R. Frisch and O. Stern, Z.<br />

Physik 85, 4 (1933).

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