Integration over regions in two or more dimensions, computing volumes and higher-dimensional totals.
IntuitionFrom slices of area to columns of volume
A single-variable integral ∫abf(x)dx chops an interval into thin segments of width Δx and sums the areas of rectangles. A double integral ∬Df(x,y)dA extends the exact same idea to a two-dimensional domain D: we tile D with tiny rectangles of area ΔA=ΔxΔy, erect a thin column of height f(xi,yj) over each tile, and let the grid refine. Adding up the columns gives the signed volume under the surface z=f(x,y), or the total mass of a plate whose surface density is f(x,y).
Interactive 3D surface plot representing the volume accumulated by a double integral over a 2D domain.
The surface z=f(x,y) over a planar domain D: the double integral ∬Df(x,y)dA accumulates the volume of vertical columns under the surface, and Fubini's theorem computes it by integrating slice by slice.
UndergraduateFormal definitions: Double and triple integrals, Fubini reduction, and Jacobians
Definition: Double and triple Riemann integrals
For a bounded function f:D⊆R2→R on a bounded measurable domain D, the double integral ∬Df(x,y)dA is the limit of Riemann sums ∑i,jf(xi∗,yj∗)ΔxiΔyj as the mesh size of the partition approaches 0. Analogously, over a solid region E⊆R3, the triple integral ∭Ef(x,y,z)dV sums over small boxes of volume ΔV=ΔxΔyΔz.
When a region is circular, cylindrical, or spherical, a smooth coordinate transformation Φ(u,v)=(x(u,v),y(u,v)) simplifies the boundary limits. Under Φ, a tiny du×dv rectangle is stretched and sheared into a parallelogram whose area is scaled by the absolute value of the Jacobian determinant ∣detDΦ∣=∂(u,v)∂(x,y). In polar coordinates (x,y)=(rcosθ,rsinθ) this factor is r, and in spherical coordinates (x,y,z)=(ρsinφcosθ,ρsinφsinθ,ρcosφ) it is ρ2sinφ.
If f(x,y) is continuous on the rectangle R=[a,b]×[c,d], then the double integral equals both iterated single integrals: ∬Rf(x,y)dA=∫ab(∫cdf(x,y)dy)dx=∫cd(∫abf(x,y)dx)dy. More generally, on a vertically simple region D={(x,y):a≤x≤b,g1(x)≤y≤g2(x)}, we have ∬Df(x,y)dA=∫ab∫g1(x)g2(x)f(x,y)dydx.
Why is it true?
Computing a volume by summing tiny boxes in a grid gives the same answer whether you first add each column along y to get cross-sectional slice areas A(x) and then integrate A(x) along x, or slice perpendicular to the y-axis first.
Proof
Partition [a,b] into m subintervals [xi−1,xi] of width Δx and [c,d] into n subintervals [yj−1,yj] of width Δy. For each fixed x, define the cross-sectional integral A(x)=∫cdf(x,y)dy. By the Mean Value Theorem for integrals, on each strip [yj−1,yj] there is yij∗∈[yj−1,yj] such that ∫yj−1yjf(xi,y)dy=f(xi,yij∗)Δy.
Summing over j=1,…,n gives A(xi)=∑j=1nf(xi,yij∗)Δy. Multiplying by Δx and summing over i=1,…,m yields ∑i=1mA(xi)Δx=∑i=1m∑j=1nf(xi,yij∗)ΔxΔy. Because f is uniformly continuous on the compact rectangle R, letting Δx,Δy→0 makes the left-hand side converge to ∫abA(x)dx=∫ab(∫cdf(x,y)dy)dx while the right-hand side converges to ∬Rf(x,y)dA. Repeating the argument with x and y swapped establishes equality with the other order of integration.
Let Φ:U→Φ(U)⊆R2 be a C1 diffeomorphism with Jacobian matrix DΦ(u,v)=(xuyuxvyv). For any integrable function f on Φ(U), we have ∬Φ(U)f(x,y)dxdy=∬Uf(x(u,v),y(u,v))∣detDΦ(u,v)∣dudv, where detDΦ=xuyv−xvyu.
Why is it true?
Just as dx=g′(u)du rescales length in one-variable substitution, ∣detDΦ(u,v)∣ measures the local area-stretching ratio when a tiny (u,v)-rectangle is mapped to an (x,y)-parallelogram.
Proof
Consider a small rectangle Rij=[ui,ui+Δu]×[vj,vj+Δv] in U. By first-order Taylor expansion around (ui,vj), the edges (Δu,0) and (0,Δv) map approximately to the tangent vectors a=Φu(ui,vj)Δu=(xu,yu)Δu and b=Φv(ui,vj)Δv=(xv,yv)Δv. The area of the parallelogram spanned by a and b in R2 equals ∣xuyv−xvyu∣ΔuΔv=∣detDΦ(ui,vj)∣ΔuΔv up to higher-order error o(ΔuΔv).
Substituting ΔAij≈∣detDΦ(ui,vj)∣ΔuΔv into the Riemann sum ∑i,jf(Φ(ui,vj))ΔAij yields ∑i,jf(Φ(ui,vj))∣detDΦ(ui,vj)∣ΔuΔv. In particular, for polar coordinates x=rcosθ, y=rsinθ, we have detDΦ=(cosθ)(rcosθ)−(−rsinθ)(sinθ)=r(cos2θ+sin2θ)=r, giving dxdy=rdrdθ.
UndergraduateReal-World Applications and Worked Examples
Multiple integrals appear across physics, probability, and engineering: in mechanics, triple integrals compute the total mass M=∭Eρ(x,y,z)dV, center of mass, and moment of inertia Iz=∭E(x2+y2)ρdV of rotating machinery; in probability and statistics, normalizing the normal distribution relies on the Gaussian integral ∫−∞∞e−x2dx=π, proved by squaring into a double integral in polar coordinates; and in astrophysics and electromagnetism, spherical integrals ρ2sinφdρdφdθ integrate gravitational and charge distributions over stars and planets.
Example: Reversing the order of integration when the inner integral has no elementary antiderivative
Evaluate the iterated integral I=∫01∫y1ex2dxdy by sketching the region of integration and reversing the order of integration via Fubini's theorem.
Solution
The inner integral ∫y1ex2dx cannot be evaluated directly in closed form because ex2 has no elementary antiderivative. However, the inequalities 0≤y≤1 and y≤x≤1 describe the triangle D={(x,y):0≤x≤1,0≤y≤x}.
By Fubini's theorem, slicing vertically first rewrites the integral as I=∫01(∫0xex2dy)dx=∫01xex2dx. Now substitute u=x2, du=2xdx to obtain I=[21ex2]01=2e−1.
Example: Evaluating the Gaussian integral via polar coordinates
Prove the Gaussian integral formula I=∫−∞∞e−x2dx=π by expressing I2 as a double integral over R2 and converting to polar coordinates.
Solution
Write the product of two independent copies of I using dummy variables x and y: I2=(∫−∞∞e−x2dx)(∫−∞∞e−y2dy)=∬R2e−(x2+y2)dxdy.
Switch to polar coordinates x=rcosθ, y=rsinθ with 0≤r<∞, 0≤θ≤2π, and Jacobian factor dxdy=rdrdθ. Then I2=∫02π∫0∞e−r2rdrdθ=2π[−21e−r2]0∞=2π⋅21=π. Since e−x2>0, taking the positive square root yields I=π.
Evaluate the double integral ∬R(2x+4y)dA over the rectangle R=[0,2]×[0,1].
When reversing the order of integration in ∫02∫x24f(x,y)dydx, which iterated integral is obtained?
In 3D spherical coordinates (x,y,z)=(ρsinφcosθ,ρsinφsinθ,ρcosφ), what is the volume element dV?
Using the Gaussian integral ∫−∞∞e−x2dx=π, what is the value of the 2D probability integral ∬R2e−(x2+y2)/2dxdy?
References
Jerrold E. Marsden, Anthony J. Tromba (2012). Vector Calculus