1.8.33 · D2Electromagnetism

Visual walkthrough — Electromagnetic waves — derivation from Maxwell's equations

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Step 0 — The three arrows we will use forever

Before any physics, meet the three actors. They are arrows (vectors) — an arrow has a length (how strong) and a direction (which way it points).

  • — the electric field arrow. Draw it blue. If a tiny positive charge sat there, it would feel a push along this arrow. Longer arrow = harder push.
  • — the magnetic field arrow. Draw it orange. It's the field a compass needle lines up with.
  • — the travel arrow (the wavevector). Green. It points the way the wave is going. Its length, written (no arrow), will later encode "how squished the ripple is". Keep this in mind: bold-arrow = direction-and-length; plain = just its length.
Figure — Electromagnetic waves — derivation from Maxwell's equations

Step 1 — The four laws, drawn as pictures

WHAT. We stand in empty space: no charges (), no currents (). Maxwell's four rules survive even here:

Term by term, in plain words:

  • — the divergence of (the dot product of with ). Read it as: "do the blue arrows spread out from this point, like water from a tap?" Equation (1) says : no taps, no drains. Field lines never start or stop in vacuum.
  • — same story for orange. (Also: no lone magnetic poles ever.)
  • — the curl of (the cross product of with ): "do the blue arrows swirl around this point, like water round a plughole?" Equation (3) says that swirl equals , i.e. a magnetic field that is changing in time makes electric arrows swirl.
  • — "how fast the orange arrow is changing per second." The minus sign is nature's direction bookkeeping (Lenz).
  • Equation (4) is the mirror: a changing electric field makes magnetic arrows swirl. The out front is the small conversion factor between the two — remember it, it becomes the speed of light.

WHY these four. (1),(2) forbid sources; (3),(4) are the coupling — each changing field births a swirl of the other. That mutual feeding is the whole engine.

Figure — Electromagnetic waves — derivation from Maxwell's equations

Step 2 — The trick: curl the swirl again

WHAT. Take equation (3) and hit both sides with another curl operator :

WHY. Look at the right side: it now contains — and equation (4) is a ready-made formula for exactly . So a second curl lets us substitute (4) into (3) and throw out entirely. Two equations tangled together become one equation about alone. This is the FaradayAmpère–Maxwell handshake.

Figure — Electromagnetic waves — derivation from Maxwell's equations

Step 3 — Untangle the left side with one identity

WHAT. There is a fixed algebraic fact, true for any arrow field :

Term by term:

  • — take the "spreading-out" number, then find its slope. The source-driven piece.
  • — the Laplacian, defined as . For a vector field it acts componentwise: . Read it as "how much does at this point differ from the average of its neighbours?" This is the curvature-in-space term — the one that shows up in every wave equation.

Apply it to , then use equation (1), :

WHY. The "no charges" law (1) erases the first term. This is the exact moment the vacuum assumption pays off — we're left with the clean curvature term only.

Figure — Electromagnetic waves — derivation from Maxwell's equations

Step 4 — Feed in Ampère–Maxwell (the right side)

WHAT. Work on the right side of Step 2. First swap the order of the space-curl and the time-derivative (allowed, the fields are smooth), then plug in equation (4):

Term by term:

  • — the swirl of , watched changing in time.
  • After (4): two time-derivatives of (the "acceleration" of the field), scaled by .

WHY. This is where vanishes for good. Everything is now written in .

Figure — Electromagnetic waves — derivation from Maxwell's equations

Step 5 — Set the two sides equal: the wave is born

WHAT. Left side (Step 3) right side (Step 4). The minus signs on both sides cancel:

Redo the whole thing starting from (4) instead of (3), using , and you get the identical shape for :

WHY it's a wave. Compare to the master Wave Equation:

  • — how curved the shape is in space.
  • — how fast the shape accelerates in time. Any quantity whose space-curvature equals its time-acceleration (up to a constant) is a travelling wave. Ours matches — so and travel.
Figure — Electromagnetic waves — derivation from Maxwell's equations

Step 6 — Plug in the numbers: it's the speed of light

WHAT. Put in the two lab constants:

WHY it's stunning. was measured with magnets and wires; was measured with static charges. Neither experiment ever involved light. Yet multiply, invert, square-root — out pops the measured speed of light. That single coincidence is what told Maxwell: light is an electromagnetic wave.

Figure — Electromagnetic waves — derivation from Maxwell's equations

Step 7 — The geometry: E, B, k form a right-handed triad

Setup convention. From here we choose our axes so the wave travels along . That means the wavevector points that way: , and from now on the plain symbol means its length only. With that choice a plane wave is:

  • , constant vector amplitudes (they carry both a size and a direction). Their magnitudes (lengths) are written and — plain, no arrow. Watch this: arrow = vector, plain = its length.
  • — the wavenumber (length of ): radians of wiggle per metre. Big = tightly squished wave.
  • — the angular frequency: radians of wiggle per second.

Three facts drop out:

  1. Transverse, from (1): . For our plane wave , so . The field has no piece along the travel direction . (See Polarization for what the remaining sideways freedom means.)
  2. , from (3): pick the surviving to lie along , so . Then Faraday's law needs . Computing the cross product with (only -derivatives survive): because . Faraday says this equals , so must point along . Hence , , : three mutually perpendicular arrows with — a right-handed set.
  3. Amplitudes, from (3): matching lengths in that same equation, , hence (lengths only).
Figure — Electromagnetic waves — derivation from Maxwell's equations

Step 8 — The degenerate case: no displacement current, no wave

WHAT. Suppose we forget Maxwell's term and use the old law in vacuum. Redo Step 4: Equating to the left side (Step 3):

WHY it matters. has no time in it — it's a static, frozen condition, not a wave. There is no travelling ripple, no , no light. So the one term Maxwell inserted is exactly the difference between a dead universe and a lit one. This is the single most important edge case in the whole story.

Figure — Electromagnetic waves — derivation from Maxwell's equations

Worked examples (each re-checked)


The one-picture summary

Figure — Electromagnetic waves — derivation from Maxwell's equations
Recall The whole walkthrough compressed into six moves

(1) Meet three arrows and one tool . (2) Write the four vacuum laws; two forbid sources, two couple and . (3) Curl Faraday's law twice so the magnetic side can be swapped in via Ampère–Maxwell. (4) The curl-of-curl identity plus collapses the left side to . (5) Ampère–Maxwell turns the right side into ; equate to get — the wave equation, whose constant reads off as m/s. (6) Feeding a plane wave back in fixes the geometry: , , mutually perpendicular, right-handed, with — and dropping Maxwell's term (Step 8) destroys the wave entirely.