The five rules of field lines become quantitative with a simple choice of convention: we establish that each field line “represents” the same amount of charge. Once this value is fixed, the field strength can be found by counting the lines, without having to solve any integral. This is the leap that turns an intuitive picture into a calculation tool.

Principle — Calculating E|\vec{E}| from the line density

Choose at a point a small surface SS_\perp perpendicular to the field lines. Let NN be the equivalent charge (in coulombs) of the lines that cross it. Then: E=4πkNS\ev{|\vec{E}| = 4\pi k\,\frac{N}{S_\perp}}

The heart of the idea is that the field strength coincides with the line density: the more crowded the lines are as they cross a given surface, the stronger the field is at that point. The surface must be perpendicular to the lines precisely so that only the lines that truly “pierce” it are counted, not the ones that graze it edge-on.

Key formula

Field lines: E=4πkNS|\vec{E}| = 4\pi k\,\frac{N}{S_\perp} where NN is the equivalent charge of the lines crossing SS_\perp, a surface perpendicular to the field.

Remember: 4πk=1/ε04\pi k = 1/\varepsilon_0.

This formula is the operational method of Faraday’s paradigm: there is no need to know either the charge QQ of the sources or the distance rr — it is enough to count the lines crossing a perpendicular surface. The constant 4πk4\pi k, which we can also write as 1/ε01/\varepsilon_0, bridges the geometry of the lines with the physical units of the field.

Example — Verification on a point charge

From a charge QQ there emerge N=QN = Q coulombs of lines (by rule 5). At distance rr, these lines spread uniformly over a sphere of area S=4πr2S_\perp = 4\pi r^2. Hence: E=4πkQ4πr2=kQr2|\vec{E}| = 4\pi k\,\frac{Q}{4\pi r^2} = k\,\frac{Q}{r^2} We recover exactly the field of the point charge: the counting formula is consistent with Coulomb’s law.

This neat consistency is no coincidence: spherical symmetry ensures that all lines cross the sphere perpendicularly and uniformly, so the density N/SN/S_\perp is the same at every point on the surface and simplifies cleanly to the expected 1/r21/r^2.

The perpendicular-surface method: we choose SS_\perp orthogonal to the field lines (in green) and count how many lines pierce it (N=7N = 7 in this example). The field is E=4πkN/S|\vec{E}| = 4\pi k\, N/S_\perp. Where the lines are denser, N/SN/S_\perp is larger, so the field is stronger.

Collegamenti

Argomenti: Campo elettrico e potenziale · Elettrostatica Concetti: Campo elettrico Competenze: Principio di sovrapposizione

Esercizi collegati: Shield and charge in a hollow conductor · Reading the field lines · Dipole and test charge