vector calculus
Divergence Theorem
You should know: surface integrals, divergence and curl
Overview
The divergence theorem (also called Gauss's theorem or Ostrogradsky's theorem) relates the flux of a vector field out of a closed surface S to the triple integral of the field's divergence over the solid region E that S encloses. It's the 3D analogue of Green's theorem, converting a (often hard) surface flux calculation into a (often easier) volume integral, or vice versa.
Interactive Graph
Formal Definition
Let E be a solid region in ℝ³ with boundary surface S = ∂E, oriented with outward-pointing normal:
Notation
| Notation | Meaning |
|---|---|
| The closed boundary surface of solid region E, with outward-pointing normal |
Theorems
Corollaries
Follows from Divergence Theorem
Worked Examples
Compute div F.
By the divergence theorem, the flux equals 3 times the volume of the ball of radius a.
Answer: 4πa³
Practice Problems
Use the divergence theorem to find the flux of F=⟨x³,y³,z³⟩ out of the sphere of radius 2 centered at the origin.
Use the divergence theorem to find the outward flux of F = ⟨x, y, z⟩ through any closed surface enclosing a volume V.
Common Mistakes
Applying the divergence theorem to a surface that isn't closed (e.g. just a hemisphere without the disk 'lid').
The divergence theorem requires S to be a CLOSED surface (the complete boundary of a solid region E). An open surface like a bare hemisphere needs Stokes' theorem instead, or must be closed off with an additional 'cap' surface before applying the divergence theorem.
Using an inward-pointing normal without adjusting the sign.
The theorem assumes OUTWARD-pointing normal on ∂E. Using an inward normal (common if a parametrization's cross product happens to point inward) flips the sign of the flux integral relative to the volume integral.
Quiz
Historical Background
The theorem was discovered independently by several mathematicians: Joseph-Louis Lagrange gave an early special case in 1762, Carl Friedrich Gauss used it in 1813 studying gravitational attraction, Mikhail Ostrogradsky proved a general form in 1826 (published 1831) while studying heat theory, and George Green stated a version in his 1828 essay. It's variously called Gauss's theorem, Ostrogradsky's theorem, or the Gauss-Ostrogradsky theorem depending on tradition, though 'divergence theorem' is the most common name in English-language calculus courses today.
- 1762
Lagrange proves an early special case
Joseph-Louis Lagrange
- 1813
Gauss applies a version of the theorem to gravitational attraction
Carl Friedrich Gauss
- 1826
Ostrogradsky proves a general form while studying heat propagation (published 1831)
Mikhail Ostrogradsky
Summary
- Divergence theorem: ∬_{∂E} F·dS = ∭_E (∇·F) dV, converting closed-surface flux to a volume integral of divergence.
- Requires a CLOSED surface ∂E with outward-pointing normal.
- If div F = 0 throughout E, net flux through any closed boundary is automatically zero (source-free/incompressible fields).
- The 3D counterpart of Green's theorem (2D) and closely related to Stokes' theorem (which relates curl flux to circulation).
References
- BookGauss, C.F. (1813). Theoria attractionis corporum sphaeroidicorum ellipticorum homogeneorum.
Mathematics