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11.7. Chirality versus Helicity 353<br />

invariance arguments. An electron is described by its energy, its momentum p,<br />

and its spin J. For spin 1/2, it is customary to use instead of the spin J the<br />

dimensionless Pauli spin operator σ; it is connected to J by<br />

σ = 2J<br />

. (11.50)<br />

�<br />

The only axial vector available is J, orσ. The operator A must therefore be<br />

proportional to σ. The axial charge operator, A0, changes sign under the parity<br />

operation as indicated by Eq. (11.46); since σ · p has this property, we set<br />

A =(A0, A), A0 =<br />

σ · p<br />

, A = σ. (11.51)<br />

mc<br />

The factor 1/mc in A0 is chosen to make the operator dimensionless.<br />

The nonrelativistic operators, as given in Eqs. (11.40) and (11.51), cannot be<br />

used for the evaluation of the muon and tau[on] decays because there all particles in<br />

the final state must be treated relativistically. The generalization of the operators<br />

V and A to relativistic leptons is well known. (17) Calculations with the relativistic<br />

operators are, however, beyond our means here, and we therefore give the transition<br />

rate for the muon decay without proof. The rate dwµ(Ee) for the emission of an<br />

electron with energy between Ee and Ee + dEe becomes, for Ee ≫ mec 2 ,<br />

dwµ(Ee) =G 2 F<br />

m2 µ<br />

4π3�7c2 E2 �<br />

e 1 − 4<br />

3<br />

Ee<br />

mµc 2<br />

�<br />

dEe. (11.52)<br />

This expression, after replacing the electron energy by the electron momentum,<br />

agrees very well with the spectrum shown in Fig. 11.7.<br />

11.7 Chirality versus Helicity<br />

• In Eq. (9.33) we gave a definition for the helicity of particles. For massive particles<br />

this quantity is not frame independent as can be seen from the fact that the dot<br />

product involves only the space-like components of the momentum so a Lorentztransformation<br />

can clearly change it. In other words, an observer moving faster<br />

than the particle would see the opposite helicity as one moving slower than the<br />

particle.<br />

In the relativistic treatment of quantum mechanics another observable emerges<br />

which is called chirality. It plays a central role in the proper definition of the<br />

currents. We don’t have the room to properly define it here, but we can make a<br />

connection to limiting cases. In particular, for highly relativistic particles (p ≫ mc)<br />

it can be shown that: (17)<br />

chirality → helicity. (11.53)<br />

17 See Halzen and Martin, Quarks and Leptons, John Wiley & Sons (1984); Chapter 5.

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