Mathematics / Calculus Multivariable & Vector Analysis 100% Free Open Access
Chapter 5 โ€ข Theory & Derivations

Unit 5: Multiple Integration: Double Integrals over General Regions & Polar Coordinates

Rigorous development of double integrals: Riemann sums, Fubini's theorem, Type I and Type II planar domains, reversing limits of integration, laminar centroids, polar sector transformations, and the Gaussian integral.

ยง5.1 Double Integrals over Rectangles & Fubini's Theorem

1. Definition via Double Riemann Sums

Let $f(x, y)$ be defined on a closed rectangle $R = [a, b] \times [c, d] = \{ (x, y) \in \mathbb{R}^2 : a \le x \le b, \; c \le y \le d \}$.

Partition $[a, b]$ into $m$ subintervals of width $\Delta x = \frac{b - a}{m}$, and $[c, d]$ into $n$ subintervals of width $\Delta y = \frac{d - c}{n}$. This divides $R$ into $m \times n$ subrectangles $R_{ij}$, each with area $\Delta A = \Delta x \Delta y$.

Choose a sample point $(x_{ij}^, y_{ij}^) \in R_{ij}$. The double Riemann sum is:

$$S_{mn} = \sum_{i=1}^m \sum_{j=1}^n f(x_{ij}^*, y_{ij}^*) \Delta A$$

Definition: If the limit exists as $m, n \to \infty$ independently of the choice of sample points, we say $f$ is integrable over $R$, and define the double integral:

$$\mathbf{\iint_R f(x, y) \, dA = \lim_{m, n \to \infty} \sum_{i=1}^m \sum_{j=1}^n f(x_{ij}^*, y_{ij}^*) \Delta A}$$

If $f(x, y) \ge 0$, the double integral represents the exact volume of the solid that lies above the rectangle $R$ and below the surface $z = f(x, y)$.


2. Fubini's Theorem on Rectangles

Evaluating a double limit of double sums directly is impractical. Guido Fubini (1907) proved that double integrals can be evaluated through two successive single-variable integrations.

Theorem (Fubini's Theorem): If $f(x, y)$ is continuous on the rectangle $R = [a, b] \times [c, d]$, then:

$$\mathbf{\iint_R f(x, y) \, dA = \int_a^b \left( \int_c^d f(x, y) \, dy \right) dx = \int_c^d \left( \int_a^b f(x, y) \, dx \right) dy}$$

That is, the double integral can be evaluated as an iterated integral in either order ($dy \, dx$ or $dx \, dy$), yielding identical results.


3. Factorization Property for Separable Integrands

If $f(x, y) = g(x) h(y)$ is separable into independent functions on $R = [a, b] \times [c, d]$:

$$\iint_R g(x) h(y) \, dA = \int_a^b g(x) \left( \int_c^d h(y) \, dy \right) dx = \left( \int_a^b g(x) \, dx \right) \left( \int_c^d h(y) \, dy \right)$$

This allows immediate factorization of 2D integrals into the product of two independent 1D integrals.

ยง5.2 Double Integrals over General Non-Rectangular Regions

Most regions of integration in applications are not rectangles. We classify bounded planar regions into two standard categories:


1. Type I Regions (Vertically Simple)

A planar region $D$ is of Type I if it lies between the vertical lines $x = a$ and $x = b$, bounded below by continuous curve $y = g_1(x)$ and above by $y = g_2(x)$:

$$D = \{ (x, y) \in \mathbb{R}^2 : a \le x \le b, \quad g_1(x) \le y \le g_2(x) \}$$

By slicing with vertical lines (integrating with respect to $y$ first):

$$\mathbf{\iint_D f(x, y) \, dA = \int_a^b \left( \int_{g_1(x)}^{g_2(x)} f(x, y) \, dy \right) dx}$$

2. Type II Regions (Horizontally Simple)

A planar region $D$ is of Type II if it lies between the horizontal lines $y = c$ and $y = d$, bounded on the left by $x = h_1(y)$ and on the right by $x = h_2(y)$:

$$D = \{ (x, y) \in \mathbb{R}^2 : c \le y \le d, \quad h_1(y) \le x \le h_2(y) \}$$

By slicing with horizontal lines (integrating with respect to $x$ first):

$$\mathbf{\iint_D f(x, y) \, dA = \int_c^d \left( \int_{h_1(y)}^{h_2(y)} f(x, y) \, dx \right) dy}$$

3. Reversing the Order of Integration

Certain integrands possess no elementary antiderivative in one variable, but become trivial when integrated in the other order (e.g., $\int e^{y^2} dy$ has no elementary form, but $\int y e^{y^2} dy$ is standard).

Procedure to Reverse Order:
  1. Extract the inequalities defining the region $D$ from the given integral limits.
  2. Sketch the geometric domain $D$ in the $xy$-plane, identifying all boundary intersections.
  3. Express the same geometric region from the opposite perspective (convert Type I to Type II, or vice versa).
  4. Re-integrate in the reversed order.

4. Physical Applications of Double Integrals

1. Planar Area: $\mathbf{A(D) = \iint_D 1 \, dA}$

2. Total Mass of a Thin Plate: If $\rho(x, y)$ is mass density: $\mathbf{M = \iint_D \rho(x, y) \, dA}$

3. Center of Mass (Centroid):

$$\bar{x} = \frac{1}{M}\iint_D x\rho(x, y) \, dA, \qquad \bar{y} = \frac{1}{M}\iint_D y\rho(x, y) \, dA$$

4. Moments of Inertia:

$$I_x = \iint_D y^2 \rho(x, y) \, dA, \quad I_y = \iint_D x^2 \rho(x, y) \, dA, \quad I_0 = I_x + I_y = \iint_D (x^2 + y^2)\rho(x, y) \, dA$$

ยง5.3 Double Integrals in Polar Coordinates and the Gaussian Integral

1. The Polar Area Differential Element

When converting from Cartesian coordinates $(x, y)$ to polar coordinates $(r, \theta)$ via $x = r\cos\theta, y = r\sin\theta$:

A polar rectangle is defined by $a \le r \le b, \alpha \le \theta \le \beta$. Consider a small polar subrectangle bounded by radius $r$ to $r + \Delta r$ and angle $\theta$ to $\theta + \Delta\theta$.

The area of this circular wedge is:

$$\Delta A = \frac{1}{2}(r + \Delta r)^2 \Delta\theta - \frac{1}{2}r^2 \Delta\theta = \frac{1}{2}(r^2 + 2r\Delta r + (\Delta r)^2 - r^2)\Delta\theta = \left( r + \frac{\Delta r}{2} \right) \Delta r \Delta\theta$$

Letting $\bar{r} = r + \frac{\Delta r}{2}$ denote the average radius, in the infinitesimal limit:

$$\mathbf{dA = r \, dr \, d\theta}$$

The Extra Factor of $r$: The factor $r$ is the Jacobian determinant of the polar coordinate transformation:

$$J = \frac{\partial(x, y)}{\partial(r, \theta)} = \begin{vmatrix} \cos\theta & -r\sin\theta \\ \sin\theta & r\cos\theta \end{vmatrix} = r\cos^2\theta + r\sin^2\theta = r$$

2. Integration Formula in Polar Coordinates

If a region $R$ is described in polar coordinates by $\alpha \le \theta \le \beta, h_1(\theta) \le r \le h_2(\theta)$:

$$\mathbf{\iint_R f(x, y) \, dA = \int_\alpha^\beta \int_{h_1(\theta)}^{h_2(\theta)} f(r\cos\theta, \; r\sin\theta) \; r \, dr \, d\theta}$$

3. Rigorous Evaluation of the Gaussian Integral

The improper Gaussian integral $I = \int_{-\infty}^\infty e^{-x^2} dx$ cannot be evaluated in single-variable calculus because $e^{-x^2}$ has no elementary antiderivative.

Theorem:

$$\mathbf{\int_{-\infty}^\infty e^{-x^2} \, dx = \sqrt{\pi}}$$
Proof:

Consider the square of the integral:

$$I^2 = \left( \int_{-\infty}^\infty e^{-x^2} \, dx \right) \left( \int_{-\infty}^\infty e^{-y^2} \, dy \right) = \int_{-\infty}^\infty \int_{-\infty}^\infty e^{-(x^2 + y^2)} \, dx \, dy$$

This represents a double integral over the entire infinite plane $\mathbb{R}^2$. Transform to polar coordinates $x^2 + y^2 = r^2$ with $0 \le r < \infty$ and $0 \le \theta \le 2\pi$:

$$I^2 = \int_0^{2\pi} \int_0^\infty e^{-r^2} (r \, dr \, d\theta) = \left( \int_0^{2\pi} d\theta \right) \left( \int_0^\infty r e^{-r^2} \, dr \right)$$
$$= 2\pi \lim_{b \to \infty} \left[ -\frac{1}{2} e^{-r^2} \right]_0^b = 2\pi \left( 0 - \left(-\frac{1}{2}\right) \right) = 2\pi \left( \frac{1}{2} \right) = \pi$$

Taking the positive square root:

$$I = \sqrt{\pi} \quad \blacksquare$$
TIERED UNIVERSITY HONORS PROBLEMS

Step-by-Step Solved Examination Problems

Comprehensive analytical derivations, multi-tier solutions (Foundational, Intermediate Exam, and Honors/Proof Challenge) with complete line-by-line verification.

Solved Problem Example 5.1: Evaluation by Reversing the Order of Integration

Evaluate the iterated integral:

$$\int_0^1 \int_x^1 \sin(y^2) \, dy \, dx$$

by reversing the order of integration.

Step 1: Identify and sketch the region of integration $D$ From the given limits:

  • Outer integral: $0 \le x \le 1$
  • Inner integral: $x \le y \le 1$

The region $D$ is bounded by:

  • $y = x$ (bottom boundary)
  • $y = 1$ (top boundary)
  • $x = 0$ (left boundary, $y$-axis)

This is a triangle with vertices at $(0, 0)$, $(0, 1)$, and $(1, 1)$.


Step 2: Express the region as Type II (horizontal slices) Viewing the triangle horizontally:

  • $y$ varies from $0$ to $1$: $0 \le y \le 1$
  • For a fixed $y$, $x$ enters at the $y$-axis ($x = 0$) and exits at the line $x = y$: $0 \le x \le y$

Step 3: Re-write and evaluate the integral

$$\int_0^1 \int_x^1 \sin(y^2) \, dy \, dx = \int_0^1 \left( \int_0^y \sin(y^2) \, dx \right) dy$$

Integrate with respect to $x$ (treating $\sin(y^2)$ as constant):

$$\int_0^y \sin(y^2) \, dx = [x \sin(y^2)]_{x=0}^{x=y} = y \sin(y^2) - 0 = y \sin(y^2)$$

Now evaluate the outer integral with respect to $y$:

$$\int_0^1 y \sin(y^2) \, dy$$

Let $u = y^2 \implies du = 2y \, dy \implies y \, dy = \frac{1}{2} du$. When $y = 0$, $u = 0$; when $y = 1$, $u = 1$:

$$\int_0^1 y \sin(y^2) \, dy = \frac{1}{2} \int_0^1 \sin(u) \, du = \frac{1}{2} [-\cos(u)]_0^1 = \frac{1}{2}(1 - \cos 1)$$
$$\mathbf{\int_0^1 \int_x^1 \sin(y^2) \, dy \, dx = \frac{1 - \cos 1}{2}} \approx 0.2298$$
Solved Problem Example 5.2: Volume of Paraboloid Solid via Polar Double Integral

Find the volume of the solid bounded above by the circular paraboloid:

$$z = 4 - x^2 - y^2$$

and bounded below by the $xy$-plane ($z = 0$).

Step 1: Determine the region of integration $R$ in the $xy$-plane The surface intersects the $xy$-plane ($z = 0$) when:

$$4 - x^2 - y^2 = 0 \implies x^2 + y^2 = 4$$

This is a circle centered at the origin with radius $R = 2$. In polar coordinates:

$$0 \le r \le 2, \qquad 0 \le \theta \le 2\pi$$

Step 2: Express the integrand in polar coordinates

$$z = 4 - (x^2 + y^2) = 4 - r^2$$

Step 3: Set up and evaluate the polar double integral Recall that $dA = r \, dr \, d\theta$:

$$V = \iint_R z \, dA = \int_0^{2\pi} \int_0^2 (4 - r^2) r \, dr \, d\theta$$
$$V = \left( \int_0^{2\pi} d\theta \right) \left( \int_0^2 (4r - r^3) \, dr \right)$$

Evaluate the independent integrals:

$$\int_0^{2\pi} d\theta = 2\pi$$
$$\int_0^2 (4r - r^3) \, dr = \left[ 2r^2 - \frac{r^4}{4} \right]_0^2 = \left( 2(4) - \frac{16}{4} \right) - 0 = 8 - 4 = 4$$

Multiply:

$$V = 2\pi \times 4 = \mathbf{8\pi} \text{ cubic units} \approx 25.133$$
Solved Problem Example 5.3: Centroid of Semicircular Lamina with Distance-Proportional Density

Find the center of mass of a semicircular lamina of radius $R$ bounded by $x^2 + y^2 \le R^2$ ($y \ge 0$), where the density at any point is directly proportional to its distance from the bounding diameter (the $x$-axis): $\rho(x, y) = k y$ ($k > 0$).

Step 1: Set up the Polar Description of the Lamina The upper semicircular region $D$ is:

$$0 \le r \le R, \qquad 0 \le \theta \le \pi$$

Since $y = r\sin\theta$, the density function is:

$$\rho = k r \sin\theta$$

Step 2: Symmetry Analysis for $\bar{x}$ The domain $D$ is symmetric with respect to the $y$-axis ($x = 0$), and the density $\rho(x, y) = ky$ is an even function of $x$ (it does not depend on $x$). Therefore, by bilateral symmetry:

$$\mathbf{\bar{x} = 0}$$

Step 3: Compute the Total Mass $M$

$$M = \iint_D \rho \, dA = \int_0^\pi \int_0^R (k r\sin\theta) (r \, dr \, d\theta) = k \left( \int_0^\pi \sin\theta \, d\theta \right) \left( \int_0^R r^2 \, dr \right)$$

Evaluate the single integrals:

$$\int_0^\pi \sin\theta \, d\theta = [-\cos\theta]_0^\pi = -(-1) - (-1) = 2$$
$$\int_0^R r^2 \, dr = \frac{R^3}{3}$$

Thus:

$$\mathbf{M = k (2) \left(\frac{R^3}{3}\right) = \frac{2k R^3}{3}}$$

Step 4: Compute the Moment about the $x$-axis $M_x$

$$M_x = \iint_D y \rho \, dA = \iint_D (r\sin\theta)(k r\sin\theta) r \, dr \, d\theta = k \int_0^\pi \int_0^R r^3 \sin^2\theta \, dr \, d\theta$$
$$M_x = k \left( \int_0^\pi \sin^2\theta \, d\theta \right) \left( \int_0^R r^3 \, dr \right)$$

Evaluate:

$$\int_0^\pi \sin^2\theta \, d\theta = \int_0^\pi \frac{1 - \cos 2\theta}{2} \, d\theta = \frac{\pi}{2}$$
$$\int_0^R r^3 \, dr = \frac{R^4}{4}$$

Thus:

$$\mathbf{M_x = k \left(\frac{\pi}{2}\right) \left(\frac{R^4}{4}\right) = \frac{k\pi R^4}{8}}$$

Step 5: Compute the Center of Mass $\bar{y}$

$$\bar{y} = \frac{M_x}{M} = \frac{\frac{k\pi R^4}{8}}{\frac{2k R^3}{3}} = \frac{k\pi R^4}{8} \cdot \frac{3}{2k R^3} = \mathbf{\frac{3\pi}{16} R}$$

Numerically, $\frac{3\pi}{16} \approx 0.589 R$. The center of mass is located at:

$$\mathbf{(\bar{x}, \bar{y}) = \left(0, \; \frac{3\pi}{16}R\right)}$$