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Multiple Integrals Reference Sheet

Verified formulas and symbol glossaries, pulled directly from each topic’s own lesson data. Unverified entries are left out rather than shown as authoritative.

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Double Integrals

Double integral as a limit of Riemann sums

Rf(x,y)dA=limm,ni=1mj=1nf(xij,yij)ΔA\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
  • R\iint_RDouble integral over the region R — add up contributions across the whole 2D region.
  • f(x,y)f(x,y)The integrand: the function whose values are being summed.
  • dAdAAn infinitesimal patch of area — the 2D equivalent of dx.
  • limm,n\lim_{m,n\to\infty}Let the grid get finer in both directions at once: more columns (m) and more rows (n).
  • i=1m\sum_{i=1}^{m}Sum over the m columns of the grid — the x-direction.
  • j=1n\sum_{j=1}^{n}Sum over the n rows of the grid — the y-direction.
  • f(xij,yij)f(x_{ij}^*, y_{ij}^*)The function's value at a sample point inside grid cell (i, j).
  • ΔA\Delta AThe area of each grid cell — the same for every cell, since the grid is uniform.
  • Δx\Delta xThe width of each grid column.
  • Δy\Delta yThe height of each grid row.

Iterated integral (rectangular region)

cdabf(x,y)dxdy\int_c^d\int_a^b f(x,y)\,dx\,dy
  • cd\int_c^dOuter integral: sweep y from c to d.
  • ab\int_a^bInner integral: sweep x from a to b, with y momentarily fixed.
  • f(x,y)f(x,y)The integrand, evaluated at each (x, y) point as the sweep proceeds.
  • dxdxIntegrate with respect to x first, holding y constant.
  • dydyThen integrate that result with respect to y.

Fubini's theorem (rectangular region)

[a,b]×[c,d]f(x,y)dA=cdabf(x,y)dxdy=abcdf(x,y)dydx\iint_{[a,b]\times[c,d]} f(x,y)\,dA = \int_c^d\int_a^b f(x,y)\,dx\,dy = \int_a^b\int_c^d f(x,y)\,dy\,dx
  • [a,b]×[c,d]\iint_{[a,b]\times[c,d]}Double integral over the rectangle formed by x in [a,b] and y in [c,d].
  • ×\timesCartesian product: pairs every x in [a,b] with every y in [c,d] to form the rectangle.
  • f(x,y)f(x,y)The same integrand throughout — Fubini's point is that its integral doesn't depend on which variable you integrate first.
  • dAdAThe area element from the double-integral definition, which the iterated integral reproduces exactly.
  • cd\int_c^dOuter integral: sweep y from c to d.
  • ab\int_a^bInner integral: sweep x from a to b, with y momentarily fixed.
  • dxdxIntegrate with respect to x, holding y constant.
  • dydyIntegrate with respect to y, holding x constant.

Double Integrals Over General Regions

Type I region

D={(x,y)axb,  g1(x)yg2(x)}D = \{(x,y) \mid a \le x \le b,\; g_1(x) \le y \le g_2(x)\}
  • a,ba, bFixed numbers — the outer x-bounds, the same for every x in the region.
  • g1(x)g_1(x)The lower boundary curve: where the region starts in y, at a given x.
  • g2(x)g_2(x)The upper boundary curve: where the region ends in y, at a given x.

Iterated integral over a Type I region

Df(x,y)dA=abg1(x)g2(x)f(x,y)dydx\iint_D f(x,y)\,dA = \int_a^b \int_{g_1(x)}^{g_2(x)} f(x,y)\,dy\,dx
  • ab\int_a^bOuter integral: sweep x over its fixed interval, exactly like a rectangle's outer bound.
  • g1(x)g2(x)\int_{g_1(x)}^{g_2(x)}Inner integral: for the current x, sweep y from the lower curve up to the upper curve.
  • dydxdy\,dxIntegrate with respect to y first, then with respect to x.

Type II region

D={(x,y)cyd,  h1(y)xh2(y)},DfdA=cdh1(y)h2(y)f(x,y)dxdyD = \{(x,y) \mid c \le y \le d,\; h_1(y) \le x \le h_2(y)\}, \qquad \iint_D f\,dA = \int_c^d \int_{h_1(y)}^{h_2(y)} f(x,y)\,dx\,dy
  • h1(y)h_1(y)The left boundary curve: where the region starts in x, at a given y.
  • h2(y)h_2(y)The right boundary curve: where the region ends in x, at a given y.

Applications of Double Integrals

Mass of a lamina

m=Dρ(x,y)dAm = \iint_D \rho(x,y)\, dA
  • ρ(x,y)\rho(x,y)Density: mass per unit area, may vary across the plate.
  • dAdAAn infinitesimal patch of area.
  • mmTotal mass of the lamina.

Moments about the x- and y-axis

Mx=Dyρ(x,y)dAMy=Dxρ(x,y)dAM_x = \iint_D y\, \rho(x,y)\, dA \qquad M_y = \iint_D x\, \rho(x,y)\, dA
  • MxM_xMoment about the x-axis — weights mass by distance from that axis (i.e. by y).
  • MyM_yMoment about the y-axis — weights mass by distance from that axis (i.e. by x).

Center of mass

xˉ=Mymyˉ=Mxm\bar{x} = \dfrac{M_y}{m} \qquad \bar{y} = \dfrac{M_x}{m}
  • xˉ,yˉ\bar{x}, \bar{y}Coordinates of the center of mass — the balance point of the plate.

Moments of inertia

Ix=Dy2ρ(x,y)dAIy=Dx2ρ(x,y)dAI0=Ix+IyI_x = \iint_D y^2\, \rho(x,y)\, dA \qquad I_y = \iint_D x^2\, \rho(x,y)\, dA \qquad I_0 = I_x + I_y
  • Ix,IyI_x, I_yMoments of inertia about the x- and y-axis — weight mass by distance squared; resistance to rotation.
  • I0I_0Polar moment of inertia, about the origin — the sum I_x + I_y.

Double Integrals in Polar Coordinates

Polar substitutions

x=rcosθ,y=rsinθ,x2+y2=r2x = r\cos\theta, \qquad y = r\sin\theta, \qquad x^2 + y^2 = r^2
  • rrdistance from the origin; the radial coordinate.
  • θ\thetaangle from the positive x-axis; the angular coordinate.
  • x=rcosθ,  y=rsinθx = r\cos\theta,\; y = r\sin\thetaCartesian-to-polar conversion.
  • x2+y2=r2x^2 + y^2 = r^2the identity that collapses circular integrands.

Area element in polar coordinates

dA=rdrdθdA = r\, dr\, d\theta
  • dA=rdrdθdA = r\,dr\,d\thetathe area element; the r is the stretch factor, not optional.

Polar region

D={(r,θ)  :  αθβ,  h1(θ)rh2(θ)}D = \{(r,\theta) \;:\; \alpha \le \theta \le \beta,\; h_1(\theta) \le r \le h_2(\theta)\}
  • [α,β][\alpha,\beta]the angular sweep of the region.
  • [h1(θ),h2(θ)][h_1(\theta), h_2(\theta)]inner and outer radial bounds.

Double integral in polar coordinates

Df(x,y)dA=αβh1(θ)h2(θ)f(rcosθ,rsinθ)  rdrdθ\iint_D 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

Area in polar coordinates

A(D)=D1dA=αβh1(θ)h2(θ)rdrdθA(D) = \iint_D 1 \, dA = \int_\alpha^\beta \int_{h_1(\theta)}^{h_2(\theta)} r\, dr\, d\theta

Surface Area

Surface area of z = f(x,y) over D

A(S)=D1+(fx)2+(fy)2dAA(S) = \iint_D \sqrt{1 + \left(f_x\right)^2 + \left(f_y\right)^2}\, dA
  • fx,fyf_x, f_yPartial derivatives of f — the surface's slopes; feed the stretch factor.
  • dAdAAn infinitesimal patch of area in the shadow region D.
  • A(S)A(S)The actual area of the surface S, not just the flat shadow D.

Triple Integrals Over a Box

Triple integral

Ef(x,y,z)dV\iiint_E f(x,y,z)\, dV
  • E\iiint_Etriple integral over the solid E.

Rectangular box

B=[a,b]×[c,d]×[p,q]B = [a,b] \times [c,d] \times [p,q]
  • [a,b],[c,d],[p,q][a,b],[c,d],[p,q]the constant bounds of a rectangular box.

Iterated triple integral over a box

BfdV=abcdpqf(x,y,z)dzdydx\iiint_B f\, dV = \int_a^b \int_c^d \int_p^q f(x,y,z)\, dz\, dy\, dx

Volume element over a box

dV=dzdydxdV = dz\,dy\,dx
  • dV=dzdydxdV = dz\,dy\,dxa little bit of volume, over a box.

Volume as a triple integral

V(E)=E1dVV(E) = \iiint_E 1\, dV

Triple integral over a general solid

EfdV=abg1(x)g2(x)h1(x,y)h2(x,y)fdzdydx\iiint_E f\, dV = \int_a^b \int_{g_1(x)}^{g_2(x)} \int_{h_1(x,y)}^{h_2(x,y)} f\, dz\, dy\, dx
  • g1(x),g2(x)g_1(x), g_2(x)middle bounds, may depend on x.
  • h1(x,y),h2(x,y)h_1(x,y), h_2(x,y)innermost bounds, may depend on x and y.

Triple Integrals in Cylindrical Coordinates

Cylindrical substitutions

x=rcosθ,y=rsinθ,z=z,x2+y2=r2x = r\cos\theta, \qquad y = r\sin\theta, \qquad z = z, \qquad x^2 + y^2 = r^2
  • r,θr, \thetapolar coordinates in the xy-plane (distance from the z-axis, angle).
  • zzheight, unchanged from Cartesian.
  • x2+y2=r2x^2+y^2=r^2collapses circular integrands.

Volume element in cylindrical coordinates

dV=rdzdrdθdV = r\, dz\, dr\, d\theta
  • dV=rdzdrdθdV = r\,dz\,dr\,d\thetavolume element; the r is the stretch factor, not optional.

Triple integral in cylindrical coordinates

EfdV=αβh1(θ)h2(θ)z1(r,θ)z2(r,θ)f(rcosθ,rsinθ,z)  rdzdrdθ\iiint_E f\, dV = \int_\alpha^\beta \int_{h_1(\theta)}^{h_2(\theta)} \int_{z_1(r,\theta)}^{z_2(r,\theta)} f(r\cos\theta, r\sin\theta, z)\; r\, dz\, dr\, d\theta
  • z1(r,θ),z2(r,θ)z_1(r,\theta), z_2(r,\theta)innermost bounds, may depend on r and θ.

Triple Integrals in Spherical Coordinates

Spherical substitutions

x=ρsinϕcosθ,y=ρsinϕsinθ,z=ρcosϕ,x2+y2+z2=ρ2x = \rho\sin\phi\cos\theta, \qquad y = \rho\sin\phi\sin\theta, \qquad z = \rho\cos\phi, \qquad x^2+y^2+z^2 = \rho^2
  • ρ\rhodistance from the origin; ρ ≥ 0.
  • ϕ\phiangle down from the positive z-axis; 0 ≤ φ ≤ π (latitude from the north pole).
  • θ\thetaangle around the z-axis in the xy-plane; 0 ≤ θ ≤ 2π (longitude).
  • x2+y2+z2=ρ2x^2+y^2+z^2=\rho^2collapses spherical integrands.

Volume element in spherical coordinates

dV=ρ2sinϕ  dρdϕdθdV = \rho^2\sin\phi\; d\rho\, d\phi\, d\theta
  • dV=ρ2sinϕdρdϕdθdV = \rho^2\sin\phi\, d\rho\, d\phi\, d\thetathe volume element; ρ²sin φ is the Jacobian, never optional.

Triple integral in spherical coordinates

EfdV=αβϕ1ϕ2ρ1ρ2fρ2sinϕ  dρdϕdθ\iiint_E f\, dV = \int_\alpha^\beta \int_{\phi_1}^{\phi_2} \int_{\rho_1}^{\rho_2} f\,\rho^2 \sin\phi\; d\rho\, d\phi\, d\theta

Change of Variables and the Jacobian

The Jacobian (2D)

(x,y)(u,v)=xuxvyuyv=xuyvxvyu\dfrac{\partial(x,y)}{\partial(u,v)} = \begin{vmatrix} \dfrac{\partial x}{\partial u} & \dfrac{\partial x}{\partial v} \\[6pt] \dfrac{\partial y}{\partial u} & \dfrac{\partial y}{\partial v} \end{vmatrix} = \dfrac{\partial x}{\partial u}\dfrac{\partial y}{\partial v} - \dfrac{\partial x}{\partial v}\dfrac{\partial y}{\partial u}
  • u,vu, vThe new coordinates you transform into.
  • (x,y)(u,v)\dfrac{\partial(x,y)}{\partial(u,v)}The Jacobian — determinant of the matrix of partial derivatives.
  • J|J|Absolute value of the Jacobian — the local area-stretch factor.

Change of variables (2D)

Rf(x,y)dA=Sf(x(u,v),y(u,v))(x,y)(u,v)dudv\iint_R f(x,y)\, dA = \iint_S f\bigl(x(u,v),\, y(u,v)\bigr)\, \left|\dfrac{\partial(x,y)}{\partial(u,v)}\right| \, du\, dv
  • RRThe original region, in the xy-plane.
  • SSThe image of R in the uv-plane, under the transformation.

Sanity check: the polar Jacobian

(x,y)(r,θ)=cosθrsinθsinθrcosθ=rcos2θ+rsin2θ=r\dfrac{\partial(x,y)}{\partial(r,\theta)} = \begin{vmatrix} \cos\theta & -r\sin\theta \\[6pt] \sin\theta & r\cos\theta \end{vmatrix} = r\cos^2\theta + r\sin^2\theta = r