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📚Calculus III

Key Concepts of Triple Integrals in Cylindrical Coordinates

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Why This Matters

Triple integrals in cylindrical coordinates are one of the most powerful tools you'll use in Calc III, and they show up constantly on exams—especially when you're dealing with regions that have circular symmetry. Think cylinders, cones, paraboloids, or any solid where the cross-section perpendicular to one axis is a circle. The moment you see phrases like "bounded by the cylinder x2+y2=4x^2 + y^2 = 4" or "region inside a cone," your brain should immediately jump to cylindrical coordinates. This isn't just about making integrals easier; it's about recognizing when and why a coordinate system matches the geometry of your problem.

You're being tested on three interconnected skills: coordinate conversion, setting up appropriate bounds, and correctly applying the Jacobian. The conceptual heart of this topic is understanding that changing coordinate systems requires adjusting your volume element—and forgetting that extra rr in dV=rdrdθdzdV = r \, dr \, d\theta \, dz is one of the most common exam mistakes. Don't just memorize the formulas below—know why each piece exists and when each technique applies.


The Coordinate System Foundation

Before you can integrate, you need to fluently move between Cartesian and cylindrical representations. These conversions form the backbone of every problem you'll encounter.

Definition of Cylindrical Coordinates (r,θ,z)(r, \theta, z)

  • rr measures radial distance—the horizontal distance from the zz-axis to the point's projection in the xyxy-plane
  • θ\theta measures angular position—the angle from the positive xx-axis, measured counterclockwise in the xyxy-plane
  • zz remains unchanged—identical to Cartesian zz, representing vertical height above or below the xyxy-plane

Conversion Formulas

  • Cartesian to cylindrical: r=x2+y2r = \sqrt{x^2 + y^2}, θ=arctan(y/x)\theta = \arctan(y/x) (adjust for quadrant), z=zz = z
  • Cylindrical to Cartesian: x=rcosθx = r\cos\theta, y=rsinθy = r\sin\theta, z=zz = z—these substitutions transform your integrand
  • Recognize common surfaces: x2+y2=a2x^2 + y^2 = a^2 becomes simply r=ar = a, which is why cylindrical coordinates excel for circular regions

Visualization of the System

  • Points live on concentric cylinders—each value of rr defines a cylinder of that radius centered on the zz-axis
  • Angular slices like pizzaθ\theta sweeps around the zz-axis, dividing space into wedge-shaped regions
  • Vertical stacking unchanged—the zz-coordinate works exactly as in Cartesian, making cylinders and cones natural to describe

Compare: Cylindrical vs. Spherical coordinates—both handle circular symmetry, but cylindrical keeps zz linear while spherical uses two angles. Use cylindrical when your region has a vertical axis of symmetry (cylinders, cones); use spherical for radial symmetry from a point (spheres, hemispheres).


The Jacobian and Volume Element

This is where students lose the most points. The volume element isn't just drdθdzdr \, d\theta \, dz—there's a critical factor that accounts for how space "stretches" in curvilinear coordinates.

Volume Element: dV=rdrdθdzdV = r \, dr \, d\theta \, dz

  • The factor rr is non-negotiable—it compensates for the fact that arc length at radius rr is rdθr \, d\theta, not just dθd\theta
  • Geometric interpretation: small volume elements farther from the zz-axis are larger, so rr scales the contribution appropriately
  • Forgetting rr is the #1 error—always write dV=rdrdθdzdV = r \, dr \, d\theta \, dz explicitly when setting up your integral

Jacobian for Cylindrical Coordinates

  • The Jacobian determinant equals rr—this comes from computing (x,y,z)(r,θ,z)\frac{\partial(x,y,z)}{\partial(r,\theta,z)} and taking the absolute value
  • Connects to the change of variables theorem—the Jacobian ensures area/volume is preserved when transforming coordinate systems
  • Appears automatically in dVdV—when you write rdrdθdzr \, dr \, d\theta \, dz, you've already incorporated the Jacobian

Compare: The Jacobian rr in cylindrical vs. ρ2sinϕ\rho^2 \sin\phi in spherical—both arise from the same principle (measuring how coordinates stretch space), but spherical has two angular variables contributing. If an FRQ asks you to justify your volume element, cite the Jacobian.


Setting Up the Integral

The art of triple integrals lies in correctly identifying bounds and choosing an efficient integration order. This is where geometric reasoning meets computational strategy.

Setting Up Triple Integrals in Cylindrical Coordinates

  • Replace all Cartesian expressions—substitute x=rcosθx = r\cos\theta, y=rsinθy = r\sin\theta, and x2+y2=r2x^2 + y^2 = r^2 throughout your integrand
  • Include the Jacobian factor rr—your integral takes the form f(r,θ,z)rdrdθdz\iiint f(r,\theta,z) \cdot r \, dr \, d\theta \, dz
  • Simplify before integrating—expressions like x2+y2\sqrt{x^2 + y^2} become simply rr, often dramatically reducing complexity

Determining Integration Limits

  • θ\theta bounds reflect angular extent—full rotation is 00 to 2π2\pi; half-space or wedge regions use smaller intervals
  • rr bounds define radial reach—typically 00 to a constant or 00 to a function of θ\theta for more complex regions
  • zz bounds capture vertical extent—often functions of rr (and sometimes θ\theta), describing top and bottom surfaces

Order of Integration

  • dzdrdθdz \, dr \, d\theta is most common—integrate vertically first when zz-bounds depend on rr, as with cones or paraboloids
  • Symmetry can eliminate variables—if the integrand is independent of θ\theta, that integral often just contributes a factor of 2π2\pi
  • Switch order strategically—if one order creates difficult bounds or integrands, try another; the region determines what's possible

Compare: Integrating a cone vs. a cylinder—for a cone like z=rz = r, your zz-bounds depend on rr (making dzdz first natural), while a cylinder r=2r = 2 has constant rr-bounds regardless of zz. Recognizing this distinction speeds up setup significantly.


Techniques and Applications

Knowing how to evaluate and when to apply cylindrical integrals separates competent students from excellent ones.

Techniques for Evaluating Triple Integrals

  • Exploit symmetry ruthlessly—odd functions integrated over symmetric intervals vanish; even functions can double half-integrals
  • Factor separable integrands—if f(r,θ,z)=g(r)h(θ)k(z)f(r,\theta,z) = g(r) \cdot h(\theta) \cdot k(z), compute three single integrals and multiply
  • Sketch the region first—a quick drawing prevents bound errors and reveals simplifications you might otherwise miss

Applications: Volume, Mass, and Center of Mass

  • Volume calculation: set f=1f = 1 and compute rdrdθdz\iiint r \, dr \, d\theta \, dz—the integral directly gives volume
  • Mass with variable density: if ρ(r,θ,z)\rho(r,\theta,z) gives density, then M=ρrdrdθdzM = \iiint \rho \cdot r \, dr \, d\theta \, dz
  • Center of mass coordinates: compute xˉ=1MxρrdV\bar{x} = \frac{1}{M}\iiint x \cdot \rho \cdot r \, dV and similarly for yˉ\bar{y}, zˉ\bar{z}—convert xx and yy to cylindrical form

Compare: Finding volume vs. finding mass—both use the same integral structure, but mass requires incorporating a density function ρ(r,θ,z)\rho(r,\theta,z). On FRQs, check whether density is constant (simplifying to volume × density) or variable (requiring full integration).


Quick Reference Table

ConceptKey Formula or Fact
Coordinate conversion (to cylindrical)r=x2+y2r = \sqrt{x^2 + y^2}, θ=arctan(y/x)\theta = \arctan(y/x), z=zz = z
Coordinate conversion (to Cartesian)x=rcosθx = r\cos\theta, y=rsinθy = r\sin\theta, z=zz = z
Volume elementdV=rdrdθdzdV = r \, dr \, d\theta \, dz
Jacobian determinantJ=rJ = r
Full rotation boundsθ[0,2π]\theta \in [0, 2\pi]
Typical rr boundsr[0,R]r \in [0, R] or r[0,f(θ)]r \in [0, f(\theta)]
Volume integralV=rdrdθdzV = \iiint r \, dr \, d\theta \, dz
Mass integralM=ρ(r,θ,z)rdrdθdzM = \iiint \rho(r,\theta,z) \cdot r \, dr \, d\theta \, dz

Self-Check Questions

  1. Why does the volume element in cylindrical coordinates include a factor of rr, and what would go wrong if you omitted it?

  2. Compare setting up bounds for a solid cylinder x2+y24x^2 + y^2 \leq 4, 0z30 \leq z \leq 3 versus a cone z=x2+y2z = \sqrt{x^2 + y^2} below z=2z = 2. How do the zz-bounds differ in structure?

  3. Given the integral (x2+y2)dV\iiint (x^2 + y^2) \, dV over a cylindrical region, what does the integrand become in cylindrical coordinates, and why does this simplify evaluation?

  4. If a density function is ρ=z\rho = z, explain how you would set up the integral for the mass of the solid bounded by r=1r = 1 and 0z40 \leq z \leq 4.

  5. When would you choose drdzdθdr \, dz \, d\theta as your integration order instead of the more common dzdrdθdz \, dr \, d\theta? Give a geometric scenario where this makes sense.