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350 The Weak Interaction<br />

The notation V ≡ (V0, V ) is a reminder that the “sandwich” ψ ∗ Vψ transforms<br />

like a four-vector. With Eqs. (11.37) and (11.38), the explicit form of V for a<br />

nonrelativistic electron is<br />

V≡(V0, V ), V0 =1, V = p<br />

. (11.40)<br />

mc<br />

There are a number of differences between the electromagnetic and weak currents.<br />

Whereas the electromagnetic current is always a neutral one that conserves charge,<br />

the weak current has a charge-changing part, J (−)<br />

w , in addition to the neutral one,<br />

J (0)<br />

w . For electrons, the corresponding weak current densities are written in analogy<br />

to the electromagnetic ones as<br />

J e(−)<br />

w<br />

= cψ ∗ eVψνe,<br />

J e(0)<br />

w = cψ∗ e Vψe, J ν(0)<br />

w = cψ∗ νe Vψνe. (11.41)<br />

The weak current is more complicated than the electromagnetic one in other ways.<br />

We have seen in chapter 9 and earlier in this chapter that the weak interaction does<br />

not respect parity. The operator V =(V0, V ) behaves under the parity operation<br />

as<br />

V0<br />

P<br />

−→ V0 V P<br />

−→ −V . (11.42)<br />

The fact that the vector part changes sign follows from Eq. (9.1). V0, on the other<br />

hand, is a probability density, and it remains unchanged under the parity operation.<br />

According to the golden rule, the transition rate for a reaction from a polarized or<br />

unpolarized source is proportional to the square of a matrix element, or<br />

��<br />

�<br />

wµ ∝ �<br />

� d 3 xψ ∗ e Vψνe · ψ ∗ νµ Vψµ<br />

�<br />

�2<br />

�<br />

� .<br />

The vector product V·V = V0V0 −V ·V remains unchanged under P ;ifw P µ denotes<br />

the transition rate after the parity operation, it is equal to wµ:<br />

w P µ<br />

= wµ.<br />

This result disagrees with the electron asymmetry observed in beta and muon decays.<br />

How can the expression for the weak current be generalized in such a way<br />

that the analogy to the electromagnetic current is not completely destroyed but that<br />

parity nonconservation is included? A hint to the answer comes from comparing<br />

linear and angular momentum. Under ordinary rotations, both behave in the same<br />

way. We have not demonstrated this fact explicitly, but the proof is straightforward<br />

if the arguments given in Section 8.2 are used. Under the parity operation, the polar<br />

vector p and the axial vector J reveal their difference: p changes sign, whereas J<br />

does not. These properties remain true for general operators V and A: V and A

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