Physical Foundations of Cosmology

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4.1 Basics 133

4.1.1 Local gauge invariance


Particles are interpreted as elementary excitations of fields. The field describing
free fermions of spin one half (for instance, electrons) obeys the Dirac equation


iγμ∂μψ−mψ= 0 , (4.1)

whereψis the four-component Dirac spinor andγμare the 4×4 Dirac matrices.
This equation can be derived from the Lorentz-invariant Lagrangian density


L=iψγ ̄ μ∂μψ−mψψ, ̄ (4.2)

whereψ ̄≡ψ†γ^0 .This Lagrangian is also invariant underglobalgauge transfor-
mations: that is, it does not change when we multiplyψby an arbitrary complex
number with unit norm, for example exp(−iθ), whereθis constant in space and
time. What happens, however, if we allowθto vary from point to point, taking
θ=eλ(xα)to be an arbitrary function of space and time? Will the Lagrangian still
remain invariant under suchlocalgauge transformation? Obviouslynot. Acting on
λ(xα), the derivative∂μgenerates an extra term,


∂μψ→∂μ(e−ieλψ)=e−ieλ(∂μ−ie(∂μλ))ψ, (4.3)

and the invariance of the original Lagrangian (4.2) can only be preserved if we
modify it by introducing an extra field. Under gauge transformations this field
should change in such a way as to cancel the extra term in (4.3). Let us consider
avector gauge field Aμand replace the derivative∂μin (4.3) with the “covariant
derivative”


Dμ≡∂μ+ieAμ. (4.4)

If we assume that under gauge transformationsAμ→A ̃μ,then


Dμψ→D ̃μ(e−ieλψ)=e−ieλ(∂μ+ieA ̃μ−ie(∂μλ))ψ.

Therefore wepostulatethe transformation law


Aμ→A ̃μ=Aμ+∂μλ, (4.5)

and find


D ̃μ(e−ieλψ)=e−ieλDμψ.

Hence


ψγ ̄ μDμψ→(ψ ̄eieλ)γμD ̃μ(e−ieλψ)=ψγ ̄ μDμψ.
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