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Classical Fields and Electromagnetism

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A classical field assigns dynamical data to every spacetime event. An action supplies bulk equations and boundary terms; constraints restrict admissible initial data; gauge freedom identifies redundant descriptions; stress-energy records what the field exchanges with matter. Electromagnetism displays all of these structures in their cleanest relativistic form.

Helpful background. Calculus and Linear Algebra for Relativity supplies variation, vector calculus, and tensor contractions; Events, Intervals, and Minkowski Geometry supplies Lorentzian geometry and index conventions; Differential Equations for Relativity supplies initial-value reasoning; the coordinate-free route uses Exterior Algebra and Differential Forms.

A finite-dimensional trajectory q(t)q(t) becomes a field ϕa(x)\phi^a(x) with one or more components at every event. The action

S[ϕ]=∫Ωd4x L(ϕa,∂μϕa,x)S[\phi]=\int_\Omega d^4x\, \mathcal L(\phi^a,\partial_\mu\phi^a,x)

has the first variation

δS=∫Ωd4x Eaδϕa+∫∂ΩdΣμ ∂L∂(∂μϕa)δϕa.\delta S =\int_\Omega d^4x\,\mathcal E_a\delta\phi^a +\int_{\partial\Omega}d\Sigma_\mu\, \frac{\partial\mathcal L} {\partial(\partial_\mu\phi^a)}\delta\phi^a.

The bulk coefficient Ea=0\mathcal E_a=0 is the Euler–Lagrange equation. The second term decides which fixed, free, or mixed boundary variations define a stationary problem. It must be retained until the boundary conditions are specified. Tong 2006–2007, §1.1, printed p. 8, PDF gives the basic field-theory integration by parts.

Electromagnetism adds a second layer. The potential AμA_\mu is redundant, but its antisymmetric curvature FμνF_{\mu\nu} is gauge-invariant. The homogeneous equation constrains that curvature, the sourced equation determines its response to current, and the antisymmetry of FF forces current conservation. Varying the same theory with respect to a background metric yields a stress-energy tensor whose divergence is the negative Lorentz force density.

This chain is the prototype used later in gauge theory and gravitation:

StructureElectromagnetic realizationQuestion it answers
ConfigurationAμA_\muWhat variables describe the field?
Gauge-invariant fieldF=dAF=dA locallyWhat can local measurements depend on?
EquationsdF=0dF=0 and d⋆F=⋆jd\star F=\star jHow does the field evolve and respond to sources?
ConstraintGauss’s lawWhich initial data are admissible?
Global datumCohomology class or U(1)U(1) holonomyHow do local potentials fit together around surfaces and loops?
Metric responseTμνT_{\mu\nu}Where are field energy and momentum stored and transferred?

This overview collects the chapter-specific consequences of the global conventions. In oriented Cartesian Minkowski coordinates,

ημν=diag⁡(−1,1,1,1),ϵ0123=+1,ϵ0123=−1.\eta_{\mu\nu}=\operatorname{diag}(-1,1,1,1), \qquad \epsilon_{0123}=+1, \qquad \epsilon^{0123}=-1.

Use rationalized Heaviside–Lorentz units and write

Aμ=(−Φ,A),Fμν=∂μAν−∂νAμ,Jμ=(ρ,J).A_\mu=(-\Phi,\mathbf A), \qquad F_{\mu\nu}=\partial_\mu A_\nu-\partial_\nu A_\mu, \qquad J^\mu=(\rho,\mathbf J).

The measured fields are defined by

F0i=−Ei,Fij=ϵijkBk.F_{0i}=-E_i, \qquad F_{ij}=\epsilon_{ijk}B^k.

These choices link the action, equations, and force:

S[A]=∫d4x(−14FμνFμν+JμAμ),∂μFμν=−Jν,∂[λFμν]=0,dpμdτ=qFμνuν.\begin{aligned} S[A] &=\int d^4x\left( -\frac14F_{\mu\nu}F^{\mu\nu}+J^\mu A_\mu \right),\\ \partial_\mu F^{\mu\nu} &=-J^\nu,\\ \partial_{[\lambda}F_{\mu\nu]} &=0,\\ \frac{dp^\mu}{d\tau} &=qF^\mu{}_{\nu}u^\nu. \end{aligned}

They reproduce

∇⋅E=ρ,∇×B−∂tE=J,\boldsymbol\nabla\mathbin{\cdot}\mathbf E=\rho, \qquad \boldsymbol\nabla\times\mathbf B-\partial_t\mathbf E=\mathbf J,

and dp/dt=q(E+v×B)d\mathbf p/dt=q(\mathbf E+\mathbf v\times\mathbf B). Different sources may reverse several definitions at once or use Gaussian or SI normalization. A consistent simultaneous translation is equivalent; changing one sign or one factor in isolation is not. Tong 2015, §§5.3.1–5.5.3, printed pp. 105–126, PDF develops the tensor, equations, force, and action in a different simultaneous convention set.

The six pages form one derivational sequence:

  1. Classical Fields and Their Actions derives the field Euler–Lagrange equation while retaining the surface term that distinguishes initial data from wall data.
  2. Maxwell’s Equations in Covariant Form builds FμνF_{\mu\nu} from the potential, recovers all four three-vector equations, and separates curl evolution from divergence constraints.
  3. Potentials, Gauge Freedom, and Constraints distinguishes local redundancy, residual gauge freedom, boundary data, and compact U(1)U(1) holonomy.
  4. Electromagnetism with Differential Forms shows which equation is metric-free, how the current becomes a three-form, and why closed need not mean globally exact.
  5. Electromagnetic Invariants and Field Classification decides when a boost removes one field, parallelizes both, or reaches the null obstruction.
  6. Lorentz Force and Electromagnetic Stress-Energy derives TμνT_{\mu\nu} by metric variation and proves local field-to-matter energy-momentum exchange.

For the coordinate-free bridge, Carroll 1997, Chapter 1, printed pp. 20–24, PDF develops the Hodge form of Maxwell’s equations, while Guillemin and Haine 2019, §§2.6, 4.6, and 5.1, Open PDF supplies local exactness, Stokes’ theorem, and de Rham cohomology.

Suppose initial data obey ∇⋅E=ρ\boldsymbol\nabla\mathbin{\cdot}\mathbf E=\rho. Use Ampère–Maxwell evolution and charge conservation to show why this constraint remains satisfied.

Solution

Take the divergence of

∇×B−∂tE=J.\boldsymbol\nabla\times\mathbf B-\partial_t\mathbf E=\mathbf J.

Because the divergence of a curl vanishes,

∂t(∇⋅E)=−∇⋅J.\partial_t(\boldsymbol\nabla\mathbin{\cdot}\mathbf E) =-\boldsymbol\nabla\mathbin{\cdot}\mathbf J.

Charge conservation gives ∂tρ=−∇⋅J\partial_t\rho=-\boldsymbol\nabla\mathbin{\cdot}\mathbf J, hence

∂t(∇⋅E−ρ)=0.\partial_t(\boldsymbol\nabla\mathbin{\cdot}\mathbf E-\rho)=0.

The constraint propagates if it holds initially. This does not make Gauss’s law optional: inconsistent initial data remain inconsistent, and a nonconserved prescribed current is incompatible with Maxwell’s equations.

At an event, let E=E0x^\mathbf E=E_0\widehat{\mathbf x} and B=0\mathbf B=0. Determine the two quadratic invariants, the field energy density and flux, and the instantaneous force and power on a stationary charge qq.

Solution

The invariants are

I=2(B2−E2)=−2E02,J=4E⋅B=0,I=2(B^2-E^2)=-2E_0^2, \qquad J=4\mathbf E\mathbin{\cdot}\mathbf B=0,

so the field is electric-dominated. Its stress-energy components give

u=12E02,S=E×B=0.u=\frac12E_0^2, \qquad \mathbf S=\mathbf E\times\mathbf B=0.

For a stationary charge, v=0\mathbf v=0, so

dpdt=qE0x^,dEparticledt=qE⋅v=0.\frac{d\mathbf p}{dt}=qE_0\widehat{\mathbf x}, \qquad \frac{dE_{\mathrm{particle}}}{dt} =q\mathbf E\mathbin{\cdot}\mathbf v=0.

The charge accelerates even though its instantaneous power is zero at that moment. If the field persists, the charge initially acquires velocity in the direction of the electric force qEq\mathbf E, so the field does positive work for either sign of nonzero qq.

After this chapter, you should be able to vary a local action with its directed surface term, translate between tensor and three-vector Maxwell equations, distinguish gauge equivalence from a physical symmetry, test a global-potential assumption, classify a field invariantly, and verify electromagnetic energy-momentum exchange.

The treatment is classical and emphasizes vacuum electrodynamics with prescribed currents or generic charged matter. Material constitutive laws, detailed radiation theory, quantum electrodynamics, and curved-spacetime propagation are outside the chapter. The next chapter, Symmetry, Conservation, and Stress-Energy, generalizes these conservation structures beyond Maxwell theory.