The covariant Maxwell equations
Recover all four Maxwell equations from tensor equations, derive current conservation from antisymmetry, and distinguish dynamical equations from potential identities.
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The question for today
What you’ll understand
- Expand the sourced tensor equation into Gauss and Ampère–Maxwell laws.
- Recover the homogeneous equations from the cyclic derivative identity.
- Explain why compatible electromagnetic sources must conserve charge.
Maxwell's four familiar vector equations become two compact spacetime statements. The compression is useful only if their content survives: source signs, displacement current, magnetic divergence, and Faraday induction must all reappear when the equations are expanded. We will check representative components and then use antisymmetry to derive a source consistency condition. This reveals that charge conservation is built into Maxwell dynamics rather than an optional assumption that can be attached to arbitrary prescribed sources afterward.
The sourced equation contains two familiar laws
Use , , , , and . Then the sourced equation is . For the temporal choice of the free index, only the spatial derivatives survive and give . Since , this is Gauss's electric law. One power of c comes from the field component and another from the current's time component; both are required.
For a spatial free index, the temporal derivative contributes minus the time derivative of E divided by c squared, while spatial derivatives produce the curl of B. Rearranging gives the Ampère–Maxwell law. The displacement-current term follows from the same tensor equation as electric Gauss law; it is not a separate correction chosen only for capacitors. In SI the common vacuum coefficients ensure the equations have one invariant propagation speed. Macroscopic material equations additionally require specified polarization, magnetization, and constitutive assumptions.
The homogeneous equation is a derivative identity
Write the second tensor statement using lower field indices: the cyclic sum of three derivatives vanishes. With three spatial indices it becomes zero magnetic divergence. With one temporal and two spatial indices it becomes Faraday's induction law, including its minus sign. This notation avoids introducing an additional orientation convention for the four-dimensional dual tensor. It uses the same lower components already established, especially , so no new field convention is hiding in the compact expression.
If for a sufficiently smooth local potential, the cyclic identity follows because mixed derivatives commute. Thus the homogeneous equations are automatically satisfied by the potential representation, while the sourced equations determine its dynamics. This argument is local; nontrivial topology can require different potential patches. Magnetic monopoles, if introduced into a different theory, would modify this homogeneous structure. We assume ordinary Maxwell electrodynamics without magnetic charge throughout the present module.
Sources and initial data must be compatible
Take another divergence of the sourced equation. The derivative pair is symmetric, while the contracted field indices are antisymmetric, so . It follows that . A proposed external current that violates local continuity cannot be a source for any solution of these Maxwell equations. Smoothness can be relaxed to distributions when derivatives are treated consistently, allowing point sources and idealized surfaces, but arbitrary inconsistency cannot be repaired by changing gauge.
There is also a useful initial-value interpretation. Electric Gauss law and zero magnetic divergence constrain an initial spatial slice, while the curl equations evolve the fields. Taking divergences of the evolution equations shows that compatible constraints remain satisfied when continuity holds. This does not remove the need for boundary conditions or supply an instantaneous action-at-a-distance solver. The tensor form guarantees consistent transformation between observers; constructing a particular physical solution still requires sources, initial data, boundaries, and an appropriate causal prescription.
Work it through
A uniform changing electric field requires current
In an ideal local region let with , and let B vanish. Find compatible rho and j using .
The electric field has no spatial dependence, so its divergence vanishes. Gauss law requires within the region, rather than a density proportional to the field's time derivative.
The magnetic curl is zero. The sourced spatial equation therefore gives . Numerically this is .
The current is spatially uniform, so its divergence is zero, consistent with stationary zero density. Faraday law also holds because both the electric curl and the magnetic time derivative vanish. The assumed local fields need external boundary and preparation conditions for a physical realization.
The compatible local sources are zero charge density and a constant current density of 17.7 microamperes per square metre along negative x.
The living notebook
Explore the model
Interactive lab · fields
Inspect source-like and curl-like geometry
For a fresh run, Reset and set BOTH q = 1 and Ω = 0; predict a radial pattern. Then Reset and set q = 0 and Ω = 1; predict a circulating pattern with no radial arrows. Inspect paused patterns or Step before relating divergence and curl to the equations.
- Fx at (1, 0)
- 0.833
- Fy at (1, 0)
- 0.5
- Field magnitude there
- 0.972
The softened illustration is q·r/(r² + 0.2) + Ω(−y, x). Moving markers indicate local direction, not integrated particle paths or a Maxwell solution. Parameter changes pause playback and recompute the model at the current elapsed time. Reset restores both parameters and returns time to zero. Playback starts paused. Adjust either parameter, then choose Play or Step.
Look forThe softened planar field separates two geometric tendencies. It does not implement electric and magnetic fields, Maxwell evolution, displacement current, or boundary conditions.
Pause & reason
Check your understanding
Your turn
Try it yourself
A static local field is with , and B = 0. Find rho and j, then check the temporal tensor equation explicitly. Use the same epsilon0 and .
Take a moment to make a prediction or work it out on paper. Open a hint when you need one.
Give me a hint
The spatial derivative of E supplies charge; a field magnitude itself does not. Use F10, not F01, in the temporal equation.
Compare with the solution
The divergence is k, so . The static zero magnetic field requires . In tensor notation . The source side is , agreeing exactly within the chosen rounded constants. The homogeneous equations hold because this electric field has zero curl and the magnetic field vanishes.
Keep the idea
Take it with you
- The sourced tensor equation combines electric Gauss law with the displacement-current equation.
- The cyclic derivative identity combines magnetic Gauss law with Faraday induction.
- Maxwell evolution admits only sources and initial constraints that satisfy local compatibility.
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