Foundations · 1888

Heaviside’s Point Charge Exploration

Length contraction wasn’t invented in 1905 — it fell out of Maxwell’s equations seventeen years earlier. In 1888, Oliver Heaviside solved for the field of a uniformly-moving point charge and found that its equipotentials are squashed into oblate ellipsoids along the direction of motion. FitzGerald (1889) and Lorentz (1892) said: if matter is held together by EM forces, and the EM forces deform this way, the matter must contract by the same factor. Einstein (1905) re-framed the contraction as kinematic — but the geometry was already there.

β = 0.60 γ = 1.250
γ 1.250 E⊥/E₀ 1.250 E∥/E₀ 0.640

① The Heaviside field

Concentric ellipses are surfaces of constant scalar potential. They squash horizontally by 1/γ as β increases. The orange rays show field strength at fixed distance — bunched perpendicular to motion, depleted along it.

The math (one line)

The scalar potential of a uniformly-moving charge is

so equipotentials satisfy — an oblate spheroid with x-semi axis and y-semi .

The electric field magnitude follows:

Two limits: (forward / backward), (sideways). The field is weaker along motion and stronger perpendicular to it.

② Bonds shrink with the field

Top: dipole at rest with bond length . Bottom: same dipole moving at β — the EM forces holding it together have deformed, and the new equilibrium spacing along motion is . Drag β to compare.

Why the rod has to contract

The attractive force between the two charges along the direction of motion scales like . For the bond to remain in mechanical equilibrium, the charges must move closer along motion by the same factor that restores the force balance. The bookkeeping (and a full calculation including all field components and self-stress) yields exactly:

This is the same formula that comes out of the kinematic derivation on the length contraction page — but here it's a consequence of Maxwell + force balance, not of postulates about spacetime.


Bonus track · separate idea

③ When the charge accelerates: radiation

The Heaviside ellipsoid is for uniform motion. If the charge accelerates, something new happens: a kink in the field lines propagates outward at exactly — this is electromagnetic radiation. The cause-and-effect speed limit baked into Maxwell's equations is the same that ends up in .

At the charge gets a brief kick (β = 0.6). Inside the inner ring () the field looks like the new uniformly-moving field, radial from the current position. Outside the outer ring () it still looks like the field of the original at-rest charge. Between the two rings: the radiation pulse — the orange kinks — moving outward at .
t = 0.00

This is the classical Purcell construction. Take-away: Maxwell already had a finite signal speed wired into it — special relativity didn't invent that, it just made the consequences geometric.

Next stops: see the kinematic derivation on the length contraction page, or watch how the constancy of forces Galilean addition to break on Galilean → Lorentz.