∞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.
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) 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) 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: radial distance from the origin
θ: polar angle measured from the positive z-axis (0≤θ≤π)
ϕ: azimuthal angle measured in the xy-plane from the positive x-axis (0≤ϕ<2π)
Coordinate transformation:
x=rsinθcosϕ
y=rsinθsinϕ
z=rcosθ
Jacobian determinant in spherical coordinates: r2sinθ
Volume element in spherical coordinates: dV=r2sinθdrdθdϕ
Spherical shells: regions bounded by two concentric spheres with radii r1 and r2
Spherical sectors: regions bounded by two meridional planes (ϕ1,ϕ2) and a cone (θ1,θ2)
Symmetry in spherical coordinates: objects with rotational symmetry about the z-axis or reflection symmetry about the xy-plane can lead to simplified integral limits
Coordinate System Breakdown
Spherical coordinates define a point in 3D space using a radial distance r, a polar angle θ, and an azimuthal angle ϕ
The radial distance r represents the distance from the origin to the point, with r≥0
The polar angle θ is measured from the positive z-axis, with 0≤θ≤π
θ=0 corresponds to the positive z-axis
θ=π/2 corresponds to the xy-plane
θ=π corresponds to the negative z-axis
The azimuthal angle ϕ is measured in the xy-plane from the positive x-axis, with 0≤ϕ<2π
ϕ=0 corresponds to the positive x-axis
ϕ=π/2 corresponds to the positive y-axis
The transformation from Cartesian to spherical coordinates is given by:
x=rsinθcosϕ
y=rsinθsinϕ
z=rcosθ
The inverse transformation from spherical to Cartesian coordinates is:
r=x2+y2+z2
θ=arccos(x2+y2+z2z)
ϕ=arctan2(y,x), where arctan2 is the two-argument arctangent function
Setting Up Triple Integrals
To set up a triple integral in spherical coordinates, follow these steps:
Identify the region of integration and its boundaries in terms of r, θ, and ϕ
Determine the order of integration (usually dr, dθ, dϕ, but it may vary depending on the region)
Write the integral with the appropriate limits of integration and the Jacobian determinant r2sinθ
Express the integrand in terms of spherical coordinates (r,θ,ϕ) if necessary
The general form of a triple integral in spherical coordinates is:
∭Ef(r,θ,ϕ)r2sinθdrdθdϕ
where E is the region of integration and f(r,θ,ϕ) is the integrand
When setting up the limits of integration, consider the following:
The radial distance r typically ranges from a minimum value r1 to a maximum value r2
The polar angle θ ranges from a minimum value θ1 to a maximum value θ2, often 0 to π
The azimuthal angle ϕ ranges from a minimum value ϕ1 to a maximum value ϕ2, often 0 to 2π
If the region has symmetry, the limits of integration may simplify:
For rotational symmetry about the z-axis, the limits for ϕ may reduce to 0 to 2π
For reflection symmetry about the xy-plane, the limits for θ may reduce to 0 to π/2
Integration Techniques
When evaluating triple integrals in spherical coordinates, use the following techniques:
Integrate with respect to r first, treating θ and ϕ as constants
Integrate with respect to θ next, treating ϕ as a constant
Integrate with respect to ϕ last
If the integrand and region of integration have symmetry, simplify the integral:
For rotational symmetry about the z-axis, the integral with respect to ϕ may simplify to a constant multiple of 2π
For reflection symmetry about the xy-plane, the integral with respect to θ may simplify to twice the integral from 0 to π/2
Use substitution or other integration techniques as needed for each variable
For integrals involving trigonometric functions of θ, substitution with u=cosθ or u=sinθ may be helpful
If the integrand is a vector-valued function F(r,θ,ϕ), integrate each component separately
Remember to include the Jacobian determinant r2sinθ in the integral
Evaluate the limits of integration in the order dϕ, dθ, dr 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 r2sinθ in the integral
Incorrectly setting up the limits of integration for r, θ, and ϕ
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 and ϕ
Remember that θ is measured from the positive z-axis, not from the xy-plane
Ensure that ϕ is measured in the xy-plane from the positive x-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 r2sinθ
If the integrand is undefined at r=0 or θ=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 (dϕ, dθ, dr) and simplify the expression
Practice Problems
Evaluate the triple integral ∭E(x2+y2+z2)dV over the sphere x2+y2+z2≤4 using spherical coordinates.
Find the volume of the region bounded by the cone z=x2+y2 and the sphere x2+y2+z2=4 using spherical coordinates.
Calculate the moment of inertia of a solid sphere of radius R and uniform density ρ about an axis through its center using spherical coordinates.
Evaluate the triple integral ∭Esin(ϕ)dV over the region E bounded by the spherical surfaces r=1, r=2, and the cone θ=π/4 using spherical coordinates.
Determine the center of mass of a solid hemisphere of radius R with density ρ(r,θ,ϕ)=kr, where k is a constant, using spherical coordinates.
Find the electric potential at a point (x,y,z) due to a charged sphere of radius R and uniform charge density ρ using spherical coordinates.
Evaluate the triple integral ∭E1+r21dV over the region E bounded by the spheres r=1 and r=2 using spherical coordinates.