Calculus IV Unit 15 – Triple Integrals in Spherical Coordinates

Triple integrals in spherical coordinates are a powerful tool for calculating volumes and other quantities in three-dimensional space. They're especially useful for objects with spherical symmetry, like spheres and ellipsoids, simplifying complex calculations by aligning the coordinate system with the object's shape. This method transforms Cartesian coordinates to spherical ones, using radial distance, polar angle, and azimuthal angle. The transformation introduces a Jacobian determinant, which is crucial for accurate integration. Mastering this technique opens doors to solving problems in physics, engineering, and advanced mathematics.

What's the Big Idea?

  • Triple integrals in spherical coordinates enable the calculation of volume, mass, and other physical quantities for three-dimensional objects with spherical symmetry
  • Spherical coordinates (r,θ,ϕ)(r, \theta, \phi) are a natural choice for objects with spherical or nearly spherical geometry, such as spheres, ellipsoids, and regions bounded by spherical surfaces
  • The transformation from Cartesian coordinates (x,y,z)(x, y, z) to spherical coordinates involves trigonometric functions and introduces a Jacobian determinant in the integral
  • Spherical coordinates simplify the integration process by aligning the coordinate system with the object's symmetry, reducing the complexity of the integral limits and integrand
  • Triple integrals in spherical coordinates have applications in physics, engineering, and mathematics, including calculating moments of inertia, electric fields, and gravitational potentials

Key Concepts

  • Spherical coordinates (r,θ,ϕ)(r, \theta, \phi):
    • rr: radial distance from the origin
    • θ\theta: polar angle measured from the positive zz-axis (0θπ)(0 \leq \theta \leq \pi)
    • ϕ\phi: azimuthal angle measured in the xyxy-plane from the positive xx-axis (0ϕ<2π)(0 \leq \phi < 2\pi)
  • Coordinate transformation:
    • x=rsinθcosϕx = r \sin\theta \cos\phi
    • y=rsinθsinϕy = r \sin\theta \sin\phi
    • z=rcosθz = r \cos\theta
  • Jacobian determinant in spherical coordinates: r2sinθr^2 \sin\theta
  • Volume element in spherical coordinates: dV=r2sinθdrdθdϕdV = r^2 \sin\theta \, dr \, d\theta \, d\phi
  • Spherical shells: regions bounded by two concentric spheres with radii r1r_1 and r2r_2
  • Spherical sectors: regions bounded by two meridional planes (ϕ1,ϕ2)(\phi_1, \phi_2) and a cone (θ1,θ2)(\theta_1, \theta_2)
  • Symmetry in spherical coordinates: objects with rotational symmetry about the zz-axis or reflection symmetry about the xyxy-plane can lead to simplified integral limits

Coordinate System Breakdown

  • Spherical coordinates define a point in 3D space using a radial distance rr, a polar angle θ\theta, and an azimuthal angle ϕ\phi
  • The radial distance rr represents the distance from the origin to the point, with r0r \geq 0
  • The polar angle θ\theta is measured from the positive zz-axis, with 0θπ0 \leq \theta \leq \pi
    • θ=0\theta = 0 corresponds to the positive zz-axis
    • θ=π/2\theta = \pi/2 corresponds to the xyxy-plane
    • θ=π\theta = \pi corresponds to the negative zz-axis
  • The azimuthal angle ϕ\phi is measured in the xyxy-plane from the positive xx-axis, with 0ϕ<2π0 \leq \phi < 2\pi
    • ϕ=0\phi = 0 corresponds to the positive xx-axis
    • ϕ=π/2\phi = \pi/2 corresponds to the positive yy-axis
  • The transformation from Cartesian to spherical coordinates is given by:
    • x=rsinθcosϕx = r \sin\theta \cos\phi
    • y=rsinθsinϕy = r \sin\theta \sin\phi
    • z=rcosθz = r \cos\theta
  • The inverse transformation from spherical to Cartesian coordinates is:
    • r=x2+y2+z2r = \sqrt{x^2 + y^2 + z^2}
    • θ=arccos(zx2+y2+z2)\theta = \arccos\left(\frac{z}{\sqrt{x^2 + y^2 + z^2}}\right)
    • ϕ=arctan2(y,x)\phi = \arctan2(y, x), where arctan2\arctan2 is the two-argument arctangent function

Setting Up Triple Integrals

  • To set up a triple integral in spherical coordinates, follow these steps:
    1. Identify the region of integration and its boundaries in terms of rr, θ\theta, and ϕ\phi
    2. Determine the order of integration (usually drdr, dθd\theta, dϕd\phi, but it may vary depending on the region)
    3. Write the integral with the appropriate limits of integration and the Jacobian determinant r2sinθr^2 \sin\theta
    4. Express the integrand in terms of spherical coordinates (r,θ,ϕ)(r, \theta, \phi) if necessary
  • The general form of a triple integral in spherical coordinates is: Ef(r,θ,ϕ)r2sinθdrdθdϕ\iiint_E f(r, \theta, \phi) \, r^2 \sin\theta \, dr \, d\theta \, d\phi where EE is the region of integration and f(r,θ,ϕ)f(r, \theta, \phi) is the integrand
  • When setting up the limits of integration, consider the following:
    • The radial distance rr typically ranges from a minimum value r1r_1 to a maximum value r2r_2
    • The polar angle θ\theta ranges from a minimum value θ1\theta_1 to a maximum value θ2\theta_2, often 0 to π\pi
    • The azimuthal angle ϕ\phi ranges from a minimum value ϕ1\phi_1 to a maximum value ϕ2\phi_2, often 0 to 2π2\pi
  • If the region has symmetry, the limits of integration may simplify:
    • For rotational symmetry about the zz-axis, the limits for ϕ\phi may reduce to 0 to 2π2\pi
    • For reflection symmetry about the xyxy-plane, the limits for θ\theta may reduce to 0 to π/2\pi/2

Integration Techniques

  • When evaluating triple integrals in spherical coordinates, use the following techniques:
    1. Integrate with respect to rr first, treating θ\theta and ϕ\phi as constants
    2. Integrate with respect to θ\theta next, treating ϕ\phi as a constant
    3. Integrate with respect to ϕ\phi last
  • If the integrand and region of integration have symmetry, simplify the integral:
    • For rotational symmetry about the zz-axis, the integral with respect to ϕ\phi may simplify to a constant multiple of 2π2\pi
    • For reflection symmetry about the xyxy-plane, the integral with respect to θ\theta may simplify to twice the integral from 0 to π/2\pi/2
  • Use substitution or other integration techniques as needed for each variable
    • For integrals involving trigonometric functions of θ\theta, substitution with u=cosθu = \cos\theta or u=sinθu = \sin\theta may be helpful
  • If the integrand is a vector-valued function F(r,θ,ϕ)\vec{F}(r, \theta, \phi), integrate each component separately
  • Remember to include the Jacobian determinant r2sinθr^2 \sin\theta in the integral
  • Evaluate the limits of integration in the order dϕd\phi, dθd\theta, drdr to obtain the final result

Real-World Applications

  • Triple integrals in spherical coordinates have numerous applications in science and engineering, including:
    • Calculating the volume of objects with spherical symmetry (spheres, ellipsoids, and regions bounded by spherical surfaces)
    • Determining the mass and center of mass of objects with non-uniform density distributions
    • Computing moments of inertia for objects rotating about an axis
    • Evaluating electric and gravitational potentials and fields for charge and mass distributions with spherical symmetry
    • Modeling heat and mass transfer in spherical systems (heat conduction in a sphere, diffusion in a spherical catalyst pellet)
  • In physics, spherical coordinates are used to describe systems with spherical symmetry:
    • Electrostatics: electric potential and field of a charged sphere or shell
    • Gravitation: gravitational potential and field of a spherical mass distribution
    • Quantum mechanics: solving the Schrödinger equation for the hydrogen atom
  • In engineering, spherical coordinates are used to analyze and design systems with spherical components:
    • Aerospace engineering: modeling the aerodynamics of spherical objects (satellites, spacecraft, and missiles)
    • Mechanical engineering: calculating the stress and strain distributions in spherical pressure vessels and bearings
    • Chemical engineering: modeling mass transfer and reaction kinetics in spherical catalyst pellets and packed bed reactors

Common Pitfalls

  • When working with triple integrals in spherical coordinates, be aware of these common pitfalls:
    • Forgetting to include the Jacobian determinant r2sinθr^2 \sin\theta in the integral
    • Incorrectly setting up the limits of integration for rr, θ\theta, and ϕ\phi
      • Make sure the limits are in the correct order and correspond to the appropriate variable
      • Ensure the limits cover the entire region of integration
    • Misinterpreting the angles θ\theta and ϕ\phi
      • Remember that θ\theta is measured from the positive zz-axis, not from the xyxy-plane
      • Ensure that ϕ\phi is measured in the xyxy-plane from the positive xx-axis
    • Incorrectly transforming the integrand from Cartesian to spherical coordinates
      • Double-check the transformation equations and simplify the expression if possible
    • Mishandling improper integrals that arise from the Jacobian determinant r2sinθr^2 \sin\theta
      • If the integrand is undefined at r=0r = 0 or θ=0\theta = 0, consider using limit evaluation or l'Hôpital's rule
    • Overlooking symmetry in the region of integration or integrand
      • Identify any rotational or reflection symmetry to simplify the integral limits or integrand
    • Improperly evaluating the limits of integration or the final result
      • Make sure to substitute the limits in the correct order (dϕd\phi, dθd\theta, drdr) and simplify the expression

Practice Problems

  1. Evaluate the triple integral E(x2+y2+z2)dV\iiint_E (x^2 + y^2 + z^2) \, dV over the sphere x2+y2+z24x^2 + y^2 + z^2 \leq 4 using spherical coordinates.

  2. Find the volume of the region bounded by the cone z=x2+y2z = \sqrt{x^2 + y^2} and the sphere x2+y2+z2=4x^2 + y^2 + z^2 = 4 using spherical coordinates.

  3. Calculate the moment of inertia of a solid sphere of radius RR and uniform density ρ\rho about an axis through its center using spherical coordinates.

  4. Evaluate the triple integral Esin(ϕ)dV\iiint_E \sin(\phi) \, dV over the region EE bounded by the spherical surfaces r=1r = 1, r=2r = 2, and the cone θ=π/4\theta = \pi/4 using spherical coordinates.

  5. Determine the center of mass of a solid hemisphere of radius RR with density ρ(r,θ,ϕ)=kr\rho(r, \theta, \phi) = kr, where kk is a constant, using spherical coordinates.

  6. Find the electric potential at a point (x,y,z)(x, y, z) due to a charged sphere of radius RR and uniform charge density ρ\rho using spherical coordinates.

  7. Evaluate the triple integral E11+r2dV\iiint_E \frac{1}{1 + r^2} \, dV over the region EE bounded by the spheres r=1r = 1 and r=2r = 2 using spherical coordinates.



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© 2024 Fiveable Inc. All rights reserved.
AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.