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Reading Time: 6 min
Last Updated: March 13, 2026
Main Ideas: 4
Reading Time: 6 min
Last Updated: March 13, 2026
Main Ideas: 4

Topic 8.6 Notes – Gauss’s Law

Verified for 2027 AP® Physics C: Electricity and Magnetism Exam
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Gauss's law connects electric flux through a closed surface to the net charge enclosed inside that surface. It gives you a powerful way to find electric fields when there's strong symmetry.

1. Gauss’s Law

Gauss’s law relates electric flux through a closed surface to the net charge enclosed:

∮E⃗⋅dA⃗=qencε0 \oint \vec{E} \cdot d\vec{A} = \frac{q_{\text{enc}}}{\varepsilon_0}

Break that apart:

  • ∮E⃗⋅dA⃗\oint \vec{E} \cdot d\vec{A} is the total electric flux through a closed surface.
  • qencq_{\text{enc}} is the net charge inside that surface.
  • ε0\varepsilon_0 is the permittivity of free space.

A Gaussian surface is any imaginary, closed 3D surface you choose to apply the law.

For example, imagine a positive point charge QQ surrounded by a spherical Gaussian surface. The electric field points radially outward everywhere, and the spherical surface encloses the charge.

Study guide illustration

Point charge with spherical Gaussian surfaces

Key properties you need solid:

  • Only enclosed charge matters. Charges outside the surface contribute zero net flux.
  • The total flux is independent of the size or shape of the surface, as long as the enclosed charge stays the same.
  • Gauss’s law is Maxwell’s first equation (electric version). The magnetic version is ∮B⃗⋅dA⃗=0\oint \vec{B}\cdot d\vec{A} = 0.

That “independent of size” idea is huge. Bigger surface means weaker field but larger area. The product stays tied to qencq_{\text{enc}}.

2. Electric Flux and Gaussian Surfaces

Electric Flux

For a small patch of surface:

E⃗⋅dA⃗=E dAcos⁡θ \vec{E} \cdot d\vec{A} = E\, dA \cos\theta

  • dA⃗d\vec{A} points outward.
  • θ\theta is the angle between E⃗\vec{E} and dA⃗d\vec{A}.

Two cases show up constantly:

  • Field perpendicular to surface → cos⁡θ=1\cos\theta = 1, flux = EdAE dA
  • Field parallel to surface → cos⁡θ=0\cos\theta = 0, flux = 0

On FRQs, they love asking why flux through certain parts is zero. If the field runs along the surface, you should immediately think “dot product is zero.”

Choosing a Smart Gaussian Surface

You’re allowed to invent the surface. Pick one that matches the symmetry:

  • Spherical symmetry → sphere
  • Cylindrical symmetry → cylinder
  • Planar symmetry → pillbox

The goal is to make:

  • EE constant over part of the surface, and/or
  • E=0E = 0 on some surfaces

Then the integral becomes simple multiplication.

If symmetry isn’t strong, Gauss’s law won’t simplify anything. That’s when you fall back on Coulomb’s law.

3. Charge Density and Enclosed Charge

If charge is spread out, you must integrate to find qencq_{\text{enc}}.

Three types:

  • Linear density
    λ=dQdx\lambda = \frac{dQ}{dx} → Q=∫λ(x) dxQ = \int \lambda(x)\, dx
  • Surface density
    σ=dQdA\sigma = \frac{dQ}{dA} → Q=∫σ dAQ = \int \sigma\, dA
  • Volume density
    ρ=dQdV\rho = \frac{dQ}{dV} → Q=∫ρ dVQ = \int \rho\, dV

Uniform cases simplify:

  • Q=λLQ = \lambda L
  • Q=σAQ = \sigma A
  • Q=ρVQ = \rho V

On tests, the hardest part is usually setting up the correct differential element. For a sphere, dV=4πr2drdV = 4\pi r^2 dr. For a cylinder, think in terms of radius and length. Geometry matters.

4. Applying Gauss’s Law to Symmetric Distributions

AP scope: point charges, spherical symmetry, cylindrical symmetry, planar symmetry.

Spherical Symmetry

Use a spherical Gaussian surface of radius rr.

Study guide illustration

Because EE is radial and constant on the sphere:

E(4πr2)=qencε0 E(4\pi r^2) = \frac{q_{\text{enc}}}{\varepsilon_0}

Results:

  • Outside any spherical distribution
    E=14πε0Qr2 E = \frac{1}{4\pi\varepsilon_0}\frac{Q}{r^2}
    It behaves like a point charge at the center.
  • Inside a uniform solid sphere
    qenc∝r3q_{\text{enc}} \propto r^3, so
    E∝rE \propto r

Students often forget this linear behavior inside.

Cylindrical Symmetry

For an infinite line with density λ\lambda, use a cylinder of radius rr and length LL.

Flux only goes through the curved surface:

E(2πrL)=λLε0 E(2\pi r L) = \frac{\lambda L}{\varepsilon_0}

E=λ2πε0r E = \frac{\lambda}{2\pi\varepsilon_0 r}

Field falls off as 1/r1/r, not 1/r21/r^2. That difference shows up in multiple-choice comparisons.

Planar Symmetry

For an infinite sheet with surface density σ\sigma, use a pillbox.

Study guide illustration

Flux comes through the two flat faces:

2EA=σAε0 2EA = \frac{\sigma A}{\varepsilon_0}

E=σ2ε0 E = \frac{\sigma}{2\varepsilon_0}

The field is constant, independent of distance. That feels strange at first but is a direct symmetry result.

Key Takeaways

Only the net enclosed charge affects total flux, even if outside charges create local fields.
If symmetry lets you treat EE as constant over a surface, Gauss’s law becomes algebra instead of calculus.
Outside a spherically symmetric distribution, the field always behaves like kQ/r2kQ/r^2.
An infinite line gives E∝1/rE \propto 1/r; an infinite sheet gives a constant EE.
When charge density is given as a function, finding qencq_{\text{enc}} usually requires integrating before applying Gauss’s law.

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Notes

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