If Maxwell’s equations follow from a perfectly Lorentz- and gauge-invariant Lagrangian, why does the straightforward Noether energy–momentum tensor look neither symmetric nor gauge invariant?

The solution has two stages: derive Maxwell’s equations, then “repair” the canonical energy–momentum tensor without changing the physical energy or momentum. This matches the indexed descriptions of parts (a) and (b).

I will use the metric ημν=diag(1,1,1,1)\eta_{\mu\nu}=\operatorname{diag}(1,-1,-1,-1).

1. The electromagnetic field as a field theory

The dynamical variable is the four-potentialAμ(x),A_\mu(x),

and the electromagnetic field tensor isFμν=μAννAμ.F_{\mu\nu} = \partial_\mu A_\nu-\partial_\nu A_\mu.

The free electromagnetic Lagrangian density isL=14FμνFμν\boxed{ \mathcal L=-\frac14F_{\mu\nu}F^{\mu\nu} }

The factor 1/41/4 compensates for the fact that the antisymmetric tensor FμνF_{\mu\nu} counts every independent component twice.


2. Part (a): Recover Maxwell’s equations

The field Euler–Lagrange equation isLAνμ(L(μAν))=0.\frac{\partial\mathcal L}{\partial A_\nu} – \partial_\mu \left( \frac{\partial\mathcal L} {\partial(\partial_\mu A_\nu)} \right)=0.

Because L\mathcal L contains AνA_\nu only through its derivatives,LAν=0.\frac{\partial\mathcal L}{\partial A_\nu}=0.

Now vary the Lagrangian:δL=12FρσδFρσ.\delta\mathcal L = -\frac12F^{\rho\sigma}\delta F_{\rho\sigma}.

SinceδFρσ=ρδAσσδAρ,\delta F_{\rho\sigma} = \partial_\rho\delta A_\sigma – \partial_\sigma\delta A_\rho,

antisymmetry of FρσF^{\rho\sigma} makes the two terms equal:δL=FρσρδAσ.\delta\mathcal L = -F^{\rho\sigma}\partial_\rho\delta A_\sigma.

Therefore,L(μAν)=Fμν.\frac{\partial\mathcal L} {\partial(\partial_\mu A_\nu)} = -F^{\mu\nu}.

The Euler–Lagrange equation becomesμ(Fμν)=0,-\partial_\mu(-F^{\mu\nu})=0,

orμFμν=0.\boxed{\partial_\mu F^{\mu\nu}=0.}

These are the source-free inhomogeneous Maxwell equations:E=0,×BEt=0.\nabla\cdot\mathbf E=0, \qquad \nabla\times\mathbf B-\frac{\partial\mathbf E}{\partial t}=0.

The other two Maxwell equations,B=0,×E+Bt=0,\nabla\cdot\mathbf B=0, \qquad \nabla\times\mathbf E+\frac{\partial\mathbf B}{\partial t}=0,

follow automatically from the definition Fμν=μAννAμF_{\mu\nu}=\partial_\mu A_\nu-\partial_\nu A_\mu. Covariantly,λFμν+μFνλ+νFλμ=0.\partial_\lambda F_{\mu\nu} +\partial_\mu F_{\nu\lambda} +\partial_\nu F_{\lambda\mu}=0.

So the important distinction is:

  • Two Maxwell equations are equations of motion.
  • The other two are identities resulting from writing F=dAF=dA.

With a current, one addsLsource=jμAμ,\mathcal L_{\text{source}}=-j_\mu A^\mu,

and obtainsμFμν=jν.\boxed{\partial_\mu F^{\mu\nu}=j^\nu.}


3. Part (b): The apparent problem with the stress-energy tensor

Translation symmetry gives the canonical Noether tensorTcanμν=L(μAλ)νAλημνL.T_{\text{can}}^{\mu\nu} = \frac{\partial\mathcal L} {\partial(\partial_\mu A_\lambda)} \partial^\nu A_\lambda -\eta^{\mu\nu}\mathcal L.

SubstitutingL(μAλ)=Fμλ,\frac{\partial\mathcal L} {\partial(\partial_\mu A_\lambda)} =-F^{\mu\lambda},

givesTcanμν=FμλνAλ+14ημνFρσFρσ\boxed{ T_{\text{can}}^{\mu\nu} = -F^{\mu\lambda}\partial^\nu A_\lambda +\frac14\eta^{\mu\nu}F_{\rho\sigma}F^{\rho\sigma} }

This tensor is conserved:μTcanμν=0.\partial_\mu T_{\text{can}}^{\mu\nu}=0.

But it has two unattractive features.

It is not manifestly gauge invariant

UnderAμAμ+μα,A_\mu\rightarrow A_\mu+\partial_\mu\alpha,

the potential-dependent term changes.

It is not symmetric

In general,TcanμνTcanνμ.T_{\text{can}}^{\mu\nu}\neq T_{\text{can}}^{\nu\mu}.

That is awkward because the physical electromagnetic stress-energy tensor should be symmetric, particularly for angular momentum conservation and coupling the theory to gravity.


4. The key freedom: conserved tensors are not unique

If TμνT^{\mu\nu} is conserved, we may add a term of the formΔTμν=λXλμν,\Delta T^{\mu\nu} = \partial_\lambda X^{\lambda\mu\nu},

whereXλμν=Xμλν.X^{\lambda\mu\nu}=-X^{\mu\lambda\nu}.

ThenμΔTμν=μλXλμν=0,\partial_\mu\Delta T^{\mu\nu} = \partial_\mu\partial_\lambda X^{\lambda\mu\nu}=0,

because the derivatives are symmetric under μλ\mu\leftrightarrow\lambda, while XX is antisymmetric.

For electromagnetism, chooseΔTμν=λ(FμλAν).\Delta T^{\mu\nu} = \partial_\lambda \left(F^{\mu\lambda}A^\nu\right).

Using the source-free equationλFμλ=0,\partial_\lambda F^{\mu\lambda}=0,

this becomesΔTμν=FμλλAν.\Delta T^{\mu\nu} = F^{\mu\lambda}\partial_\lambda A^\nu.

Add it to the canonical tensor:Tμν=FμλνAλ+FμλλAν+14ημνF2.T^{\mu\nu} = -F^{\mu\lambda}\partial^\nu A_\lambda + F^{\mu\lambda}\partial_\lambda A^\nu + \frac14\eta^{\mu\nu}F^2.

Combine the first two terms:Fμλ(λAννAλ)=FμλFνλ.F^{\mu\lambda} \left( \partial_\lambda A^\nu-\partial^\nu A_\lambda \right) = -F^{\mu\lambda}F^\nu{}_{\lambda}.

Thus the improved tensor isTEMμν=FμλFνλ+14ημνFρσFρσ\boxed{ T_{\mathrm{EM}}^{\mu\nu} = -F^{\mu\lambda}F^\nu{}_{\lambda} + \frac14\eta^{\mu\nu} F_{\rho\sigma}F^{\rho\sigma} }

This is the standard electromagnetic stress-energy tensor.


5. Why this is the correct physical answer

The improved tensor has all the desired properties:TEMμν=TEMνμ,T_{\mathrm{EM}}^{\mu\nu}=T_{\mathrm{EM}}^{\nu\mu},

it is gauge invariant because it depends only on FμνF_{\mu\nu}, and it remains conserved:μTEMμν=0.\partial_\mu T_{\mathrm{EM}}^{\mu\nu}=0.

Its components have familiar physical meanings:T00=12(E2+B2)T^{00} = \frac12\left(\mathbf E^2+\mathbf B^2\right)

is the electromagnetic energy density, whileT0i=(E×B)iT^{0i}=(\mathbf E\times\mathbf B)^i

is the energy flux or momentum density—the Poynting vector. The spatial components areTij=EiEjBiBj+12δij(E2+B2),T^{ij} = -E_iE_j-B_iB_j + \frac12\delta^{ij} \left(\mathbf E^2+\mathbf B^2\right),

which describe electromagnetic pressure and shear stress.

The added divergence does not change the total four-momentumPν=d3xT0ν,P^\nu=\int d^3x\,T^{0\nu},

provided the fields vanish sufficiently rapidly at spatial infinity. It changes the local bookkeeping, not the total conserved quantities.

The real lesson of Problem 2.1

This problem is teaching three foundational QFT ideas:

  1. Fields are obtained by applying the Euler–Lagrange principle to a Lagrangian density, just as particle equations follow from an ordinary Lagrangian.
  2. Noether currents are not unique. You may add identically conserved “improvement terms.”
  3. The naïve Noether tensor is not always the most physically useful representative. For gauge fields, it must be improved to make gauge invariance and symmetry manifest.

In one line:Canonical Noether tensor+harmless total divergence=physical electromagnetic stress-energy tensor.\boxed{ \text{Canonical Noether tensor} + \text{harmless total divergence} = \text{physical electromagnetic stress-energy tensor}. }