Engineering Math Practice

Triple Integrals in Cylindrical Coordinates

Convert a triple integral over a solid cylinder to cylindrical coordinates and evaluate it.

The idea. Cylindrical coordinates are just polar coordinates with a z-axis bolted on. You already know two-thirds of this from polar integrals — convert x, y to r, θ exactly as in polar, leave z alone:

x=rcosθ,y=rsinθ,z=z,x2+y2=r2x = r\cos\theta, \qquad y = r\sin\theta, \qquad z = z, \qquad x^2 + y^2 = r^2

Cylindrical substitutions

  • r,θr, \thetapolar coordinates in the xy-plane (distance from the z-axis, angle).
  • zzheight, unchanged from Cartesian.
  • x2+y2=r2x^2+y^2=r^2collapses circular integrands.

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The volume element:

dV=rdzdrdθdV = r\, dz\, dr\, d\theta

Volume element in cylindrical coordinates

  • dV=rdzdrdθdV = r\,dz\,dr\,d\thetavolume element; the r is the stretch factor, not optional.

The r is back, and it's the same trap as polar. The volume element carries an r — it's r dz dr dθ, never dz dr dθ. Same geometric reason: a cylindrical wedge is wider the farther out you go. If you internalized the forgotten-r from polar integrals, you already have this; it just rides along in 3D.

When to reach for cylindrical — the tell: the solid has circular symmetry around the z-axis. Cylinders, cones, paraboloids, anything round in the xy-plane that extends up and down. Or the integrand has x² + y² in it, which collapses to r². Same signal as polar, plus a vertical dimension.

The general form:

EfdV=αβh1(θ)h2(θ)z1(r,θ)z2(r,θ)f(rcosθ,rsinθ,z)  rdzdrdθ\iiint_E f\, dV = \int_\alpha^\beta \int_{h_1(\theta)}^{h_2(\theta)} \int_{z_1(r,\theta)}^{z_2(r,\theta)} f(r\cos\theta, r\sin\theta, z)\; r\, dz\, dr\, d\theta

Triple integral in cylindrical coordinates

  • z1(r,θ),z2(r,θ)z_1(r,\theta), z_2(r,\theta)innermost bounds, may depend on r and θ.

The bounds nest inside-out just like rectangular triples: the z-bounds (innermost) can depend on r and θ; the r-bounds can depend on θ; the θ-bounds are constants.

Worked example

EzdV,E:x2+y21,  0z2\iiint_E z\, dV, \qquad E: x^2+y^2 \le 1,\; 0 \le z \le 2
  1. x2+y21,  0z2    0θ2π,  0r1,  0z2x^2+y^2 \le 1,\; 0 \le z \le 2 \;\Longrightarrow\; 0 \le \theta \le 2\pi,\; 0 \le r \le 1,\; 0 \le z \le 2

    Convert the region. Circular in the xy-plane, radius 1: θ from 0 to 2π, r from 0 to 1. The z bounds are given: 0 to 2. Convert the integrand: f = z has no x or y, so it stays z.

  2. 02π0102zrdzdrdθ\int_0^{2\pi} \int_0^1 \int_0^2 z \cdot r\, dz\, dr\, d\theta

    Set up — attach the r.

  3. 02zdz=z2202=202π012rdrdθ\int_0^2 z\, dz = \frac{z^2}{2}\bigg|_0^2 = 2 \quad\Longrightarrow\quad \int_0^{2\pi}\int_0^1 2r\, dr\, d\theta

    Innermost, over z.

  4. 012rdr=r201=102π1dθ\int_0^1 2r\, dr = r^2\big|_0^1 = 1 \quad\Longrightarrow\quad \int_0^{2\pi} 1\, d\theta

    Middle, over r.

  5. 02π1dθ=2π\int_0^{2\pi} 1\, d\theta = 2\pi

    Outermost, over θ. Notice how the r from dV made the middle integral 2r, not 2 — miss it and you'd get a wrong answer that still looks plausible.

Answer:

2π2\pi

How to solve one of these

  1. 1.

    Spot the circular symmetry around the $z$-axis, or $x^2+y^2$ in the integrand. That's the signal to use cylindrical.

  2. 2.

    Convert the $xy$-part to polar. Find the θ\theta sweep and the rr bounds exactly as in ordinary polar coordinates. Leave zz as zz.

  3. 3.

    Find the $z$-bounds. Often given directly, or the surfaces the solid sits between — they may depend on rr.

  4. 4.

    Convert the integrand. Every xrcosθx \to r\cos\theta, yrsinθy \to r\sin\theta, x2+y2r2x^2+y^2 \to r^2; zz stays.

  5. 5.

    Attach the $r$. Write rdzdrdθr\,dz\,dr\,d\theta. Multiply it in before integrating.

  6. 6.

    Integrate inside-out. zz, then rr, then θ\theta. Substitute bounds at each step.

EfdV=αβh1(θ)h2(θ)z1(r,θ)z2(r,θ)f(rcosθ,rsinθ,z)  rdzdrdθ\iiint_E f\, dV = \int_\alpha^\beta \int_{h_1(\theta)}^{h_2(\theta)} \int_{z_1(r,\theta)}^{z_2(r,\theta)} f(r\cos\theta, r\sin\theta, z)\; r\, dz\, dr\, d\theta

Convert x and y to r and θ exactly as in polar, leave z alone, integrate innermost to outermost — z, then r, then θ — and multiply by r dz dr dθ.

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