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Subatomic Physics

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388 Introduction to Gauge Theories<br />

ϕ1 = e<br />

�<br />

A·dx, ϕ2 =<br />

�c s1<br />

e<br />

�<br />

A·dx. (12.16)<br />

�c s2<br />

The interference pattern observed on the screen is determined by the phase difference<br />

of the two waves. If |s1| = |s2|, so that P is located at equal distances from<br />

the two slits, the phase difference δϕ is<br />

δϕ = ϕ1 − ϕ2 = e<br />

�� � �<br />

A·dx − A·dx<br />

�c s1<br />

s2<br />

= e<br />

�<br />

A·dx =<br />

�c<br />

e<br />

Φ. (12.17)<br />

�c<br />

Thus, even though there is no magnetic field along the paths of the electrons, they<br />

show interference effects that depend on, and vary with the vector potential A,<br />

which therefore acquires a physical reality that was absent in classical mechanics.<br />

The effect occurs because the local phase at two space–time points is connected<br />

by the potential. The importance of potentials in quantum theory was stressed by<br />

Aharonov and Bohm (2) and the phase difference dependence on the vector potential<br />

A has been observed. (3)<br />

It was shown by Berry (4) that the Aharonov–Bohm effect is a special case of a<br />

geometric phase present for any system transported adiabatically (slowly) around<br />

a closed circuit. The phase can be made visible by beating the system that is made<br />

to go around the circuit with the same system made to go straight to the detector;<br />

another way is to examine the superposition of stationary spin states of a system<br />

of particles, such as neutrons, before and after they have completed a closed path,<br />

as in a helical magnetic field. Berry makes a classical analogy to a body moving<br />

around a closed path on a curved surface. Thus, if a matchstick is taken around a<br />

closed path on a plane, without rotating it, it points in the same direction at the<br />

end as at the start. If, however, it is taken around a path on a sphere, such as from<br />

the North pole of the Earth to the equator, then taken to a different longitude and<br />

returned to the North pole, it ends up pointing along a different longitude at the<br />

end than at the start. Like the quantum mechanical effect, the change in direction<br />

only depends on geometrical factors.<br />

12.3 Gauge Invariance for Non-Abelian Fields<br />

The electromagnetic field is a simple example of a gauge field. If we are to include<br />

the weak interactions, then there are two problems that need to be solved. The first<br />

one is that both neutral and charged vector bosons are required. The second one<br />

is that the weak bosons W + and Z 0 are massive, whereas we showed that gauge<br />

invariance requires massless fields. We tackle the first problem in this section.<br />

3 R. G. Chambers, Phys. Rev. Lett. 5, 3 (1960).<br />

4 V. M. Berry, Proc. R. Soc. London A392, 45 (1984); Sci. Amer. 259, 46 (December 1988).

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