Potential of Continuous Distributions
Chapter 1 — Electrostatics
Because potential is a scalar, computing \(V\) from a charge distribution is almost always easier than computing \(\vec E\) directly — no component-by-component bookkeeping, no cancellations to track. Once you have \(V(\vec r)\), you can get the field (if you need it) via \(\vec E = -\nabla V\).
Master formula
For any charge distribution (volume, surface, or line),
\[V(\vec r) = \frac{1}{4\pi\epsilon_0}\int \frac{dq'}{|\vec r - \vec r\,'|}.\]
With the convention \(V(\infty) = 0\). For volume, \(dq' = \rho(\vec r\,')\,dV'\); for surface, \(dq' = \sigma\,dA'\); for line, \(dq' = \lambda\,d\ell'\).
Two strategies
Direct integration: Plug in \(dq\) and compute. Works whenever you can write down the integral in coordinates aligned with the distribution's symmetry.
Field-first, then line integral: If you already know \(\vec E\) from Gauss's law (sphere, line, plane), use
\[V(\vec r) = V(\vec r_0) - \int_{\vec r_0}^{\vec r} \vec E\cdot d\vec \ell.\]
Pick a convenient reference point and integrate along a convenient path.
Worked examples
Ring of charge (radius \(R\), total \(Q\)): on the axis at height \(z\), every element is at the same distance \(\sqrt{R^2 + z^2}\), so
\[V(z) = \frac{1}{4\pi\epsilon_0}\frac{Q}{\sqrt{R^2 + z^2}}.\]
Spherical shell of radius \(R\), total \(Q\): integrating \(\vec E\) inward from infinity,
\[V(r) = \begin{cases}\dfrac{kQ}{r} & r \ge R,\\ \dfrac{kQ}{R} & r < R.\end{cases}\]
\(V\) is constant inside (since \(\vec E = 0\)) and continuous at the surface.
Uniform solid ball of radius \(R\), total \(Q\): outside, same as point charge. Inside, integrate \(E = kQr/R^3\) from \(R\) to \(r\):
\[V(r) = \frac{kQ}{2R}\left(3 - \frac{r^2}{R^2}\right),\quad r < R.\]
Max at the center: \(V(0) = \tfrac{3}{2}kQ/R\).
Disks, rods, and other finite shapes
For finite geometries (rod of length \(L\), disk of radius \(R\)), \(V\) along a symmetry axis typically integrates cleanly:
\[V_{\text{disk}}(z) = \frac{\sigma}{2\epsilon_0}\left(\sqrt{R^2+z^2}-|z|\right)\]
along the axis of a uniformly charged disk. Take \(R\to\infty\) to recover the (reference-dependent) linear result for an infinite plane. Differentiating with respect to \(z\) reproduces the disk's axial \(E\) — a nice consistency check.
Practice Problems
Hint
Solution
\(V = kQ/R\). Note \(\vec E = 0\) at the same point.
Answer: \(V = kQ/R\).
Hint
Solution
\(V = k\lambda \int_0^L \frac{dx'}{x_0-x'} = k\lambda \ln\frac{x_0}{x_0 - L}\).
Answer: \(V = k\lambda \ln\dfrac{x_0}{x_0-L}\).
Hint
Solution
\(V(r) = -\int_\infty^r kQ/r'^2\,dr' = kQ/r\).
Answer: \(V(r) = kQ/r\) for \(r > R\). Same as a point charge.
Hint
Solution
\(V = 2\pi k \sigma \int_0^R \frac{r\,dr}{\sqrt{r^2+z^2}} = 2\pi k\sigma[\sqrt{r^2+z^2}]_0^R = \frac{\sigma}{2\epsilon_0}(\sqrt{R^2+z^2} - z)\).
Answer: \(V(z) = \dfrac{\sigma}{2\epsilon_0}(\sqrt{R^2+z^2} - z)\). Differentiating gives the disk's axial \(E\).