Skip to content
Free public beta until December 4, 2026: every course is open, no card needed. After that, the first chapter of each course stays free and full access is a one-time $39 ($19 for up to 100 founding members chosen for helpful feedback). Your progress is kept. How the beta works

Recipe

Apply the Divergence Theorem to a closed-surface flux integral

Use when: you need \oiint_S\mathbf{F}\cdot d\mathbf{S} for a closed surface S fully enclosing a solid E

Goal: the flux value, computed as a triple integral of divergence over E instead of a surface integral over S

Taught in The divergence theorem

  1. 1

    Check that S fully encloses a solid E with no boundary rim, and that its stated orientation is outward.

    Why: the Divergence Theorem needs a genuinely closed surface; an open surface with a rim needs Stokes' Theorem instead, not this one.

  2. 2

    Write \mathbf{F}=(P,Q,R) and identify the solid region E that S encloses.

    Example

    Let \mathbf{F}=(x^2,\,y^2,\,z^2) and let S be the boundary of the box E=[0,1]\times[0,2]\times[0,3], outward-oriented.

    Why: the theorem trades the surface's flux for an integral over exactly this solid.

  3. 3

    Differentiate each component with respect to its own matching variable, then add all three.

    Example

    P_x=2x, Q_y=2y, R_z=2z, so \operatorname{div}\mathbf{F} = 2x+2y+2z.

    Why: this is the volume-density of outward flux that the theorem integrates over E.

  4. 4

    Integrate \operatorname{div}\mathbf{F} over E, choosing coordinates that match E's shape.

    • E is a ball or built from spheres — spherical coordinates usually simplify the integral.
    • E is a cylinder or has circular cross-sections — cylindrical coordinates usually simplify it.
    • E is a box or another axis-aligned solid — rectangular coordinates are usually simplest.

    Why: the theorem only supplies the integrand; picking coordinates that match E's shape is what makes the triple integral tractable.

  5. 5

    Carry out the integration over E's actual bounds. This is the final flux value.

    Example

    \displaystyle\iiint_E (2x+2y+2z)\,dV = \int_0^1\!\!\int_0^2\!\!\int_0^3 (2x+2y+2z)\,dz\,dy\,dx = 36.

    Why: this number equals the original closed-surface flux integral exactly, with no surface parametrization ever required.

Common mistakes

  • Applying this theorem to a surface that is not actually closed, such as one with a rim.
  • Forgetting that the standard theorem assumes outward orientation, which needs a sign flip if the surface is oriented inward.
  • Computing divergence from only one or two components instead of summing all three matching partials.
  • Choosing coordinates that fight the solid's natural shape, turning an easy integral into a hard one.