Triple Integral Definition and Applications
Consider the iterated integral $$\ds \int_{-3}^3
\int_0^{\sqrt{9-y^2}}\int_0^{9-x^2-y^2} dzdxdy.$$ This is an
integral of the form $\iiint_D dV$, which means along some
solid region $D$ in the plane, we are adding up little bits of
volume. This integral should give the volume of some solid
region in space. Sketch the region $D$ in space. Compute the
inside integral, and compare this to the first problem in the
double integral unit. Then evaluate the remaining integrals
(though you might want to change coordinate systems before
doing so).
When working with double integrals, there were two
different ways to set up the bounds for our integrals, as
$dA=dxdy=dydx$. When working with triple integrals, there are six
different ways to set up the bounds for our integrals, as
$$dV=dxdydz = dxdzdy = dydxdz=dydzdx=dzdxdy=dzdydx.$$
Consider again the iterated integral $$\ds \int_{-3}^3
\int_0^{\sqrt{9-y^2}}\int_0^{9-x^2-y^2} dzdxdy.$$ There are 5
other iterated integrals that are equal to this integral, by
switching the order of the bounds. One of the integrals is
$\int_0^9\int_0^{\sqrt{9-z}}\int_{-\sqrt{9-x^2-z}}^{\sqrt{9-x^2-z}}
dydxdz$. Set up the equivalent integrals using the bound
$dydzdx$ and $dxdzdy$. We'll look at the remaining 2 in class
(though you're welcome to finish them and present them with
your work).
Consider the iterated integral
$$\int_{-1}^1\int_0^{1-x^2}\int_0^{y} dzdydx.$$ The bounds for
this integral describe a region in space which satisfies the 3
inequalities $-1\leq x\leq 1$, $0\leq y\leq 1-x^2$, and $0\leq
z\leq y$.
- Draw the solid domain $D$ in space described by the
bounds of the iterated integral.
- There are 5 other iterated integrals equivalent to this
one. Set up the integrals that use the bounds $dydxdz$ and
$dxdzdy$. We'll create the other 3 in class (though you are
welcome to include them as part of your presentation).
In each problem below, you'll be given enough information to
determine a solid domain $D$ in space. Draw the solid $D$ and
then set up an iterated integral (pick any order you want) that
would give the volume of $D$. You don't need to evaluate the
integral, rather you just need to set them up.
- The region $D$ under the surface $z=y^2$, above the
$xy$-plane, and bounded by the planes $y=-1$, $y=1$, $x=0$,
and $x=4$.
- The region $D$ in the first octant that is bounded by the
coordinate planes, the plane $y+z=2$, and the surface
$x=4-y^2$.
- The pyramid $D$ in the first octant that is below the
planes $\ds\frac{x}{3}+\frac{z}{2}=1$ and
$\ds\frac{y}{5}+\frac{z}{2}=1$. [Hint, don't let $z$ be the
inside bound.]
- The region $D$ that is inside both right circular
cylinders $x^2+z^2=1$ and $y^2+z^2=1$.
We can find average value, centroids, centers of mass,
moments of inertia, and radii of gyration exactly as before, We
just now need to integrate using three integrals, and replace
$ds$, $dA$ or $d\sigma$, with $dV$.
Consider the triangular wedge $D$ that is in the first octant,
bounded by the planes $\ds\frac{y}{7}+\frac{z}{5}=1$ and
$x=12$. In the $yz$ plane, the wedge forms a triangle that
passes through the points $(0,0,0)$, $(0,7,0)$, and $(0,0,5)$.
Set up integral formulas that would give the centroid $(\bar
x,\bar y, \bar z)$ of $D$. Actually compute the integrals for
$\bar y$. Then state $\bar x$ and $\bar z$ by using symmetry
arguments.
Consider the tetrahedron $D$ in the first octant that is
underneath the plane that intersects the coordinate axes in the
three point $(a,0,0)$, $(0,b,0)$ and $(0,0,c)$, where you can
assume that $a,b,c>0$.
- An equation of an ellipse that passes through $(a,0)$ and
$(0,b)$ is $\ds\frac{x^2}{a^2}+\frac{y^2}{b^2}=1$. An
equation of a line through these same two points is
$\ds\frac{x}{a}+\frac{y}{b}=1$. An equation of an ellipsoid
through the three points $(a,0,0)$, $(0,b,0)$, and $(0,0,c)$
is $\ds\frac{x^2}{a^2}+\frac{y^2}{b^2}+\frac{z^2}{c^2}=1$.
Guess an equation of the plane through these same three
points, and then verify that your guess is correct by
plugging the 3 points into your equation. This will provide
you with an extremely fast way to get an equation of a
plane.
- Set up an iterated integral that would give the volume of
$D$.
- If the density is $\delta(x,y,z) = 3x+2yz$, set up
iterated integrals that would give the mass $m$ and moment of inertia $I_y$ about the
$y$-axis.
Changing Coordinate Systems: The Jacobian
Just as we did
with polar coordinates in two dimensions, we can compute a
Jacobian for any change of coordinates in three dimensions. We
will focus on cylindrical and spherical coordinate systems.
Remember that the Jacobian of a transformation is found by first
taking the derivative of the transformation, then finding the
determinant, and finally computing the absolute value.
The cylindrical change of coordinates is
$$x=r\cos\theta,y=r\sin\theta, z=z, \text{ or in vector form }
\vec C(r,\theta,z) = (r\cos\theta,r\sin\theta, z).$$ The
spherical change of coordinates is \begin{align*}
x=\rho\sin\phi\cos\theta,y&=\rho\sin\phi\sin\theta,
z=\rho\cos\phi, \quad \text{or in vector form}\\ \vec
S(\rho,\phi,\theta) &=
(\rho\sin\phi\cos\theta,\rho\sin\phi\sin\theta,\rho\cos\phi).
\end{align*}
- Verify that the Jacobian of the cylindrical
transformation is
$\ds\frac{\partial(x,y,z)}{\partial(r,\theta,z)} = |r|$. If
you want to make sure you don't have to use absolute values,
what must you require?
- The Jacobian of the spherical transformation is
$\ds\frac{\partial(x,y,z)}{\partial(\rho,\phi,\theta)} =
|\rho^2\sin\phi|$. If you want to make sure you don't have to
use absolute values, what must you require?
The previous problem shows us that we can write $$dV=dxdydz
= rdrd\theta dz = \rho^2\sin\phi d\rho d\phi d\theta,$$ provided
we require $r\geq0$ and $0\leq \phi\leq \pi$. Cylindrical
coordinates are extremely useful for problems which involve
cylinders, paraboloids, and cones. Problems which involve cones
and spheres often have simple integrals in spherical coordinates.
% The double cone $z^2=x^2+y^2$ has two halves. Each half
is called a nappe. Set up an integral in the coordinate system
of your choice that would give the volume of the region that is
between the $xy$ plane and the upper nappe of the double cone
$z^2=x^2+y^2$, and between the cylinders $x^2+y^2=4$ and
$x^2+y^2=16$. Then evaluate the integral.
Set up an integral in the coordinate system of your choice that
would give the volume of the solid ball that is inside the
sphere $a^2=x^2+y^2+z^2$. Compute the integral to give a
formula for the volume of a sphere of radius $a$. Then set up (don't evaluate) an iterated integral that
would give the moment of inertia $I_x$ about the $x$-axis, if
the density is a constant, so $\delta =c$.
% Find the volume of the solid domain $D$ in space which
is above the cone $z=\sqrt{x^2+y^2}$ and below the paraboloid
$z=6-x^2-y^2$. Use cylindrical coordinates to set up and then
evaluate your integral. You'll need to find where the surface
intersect, as their intersection will help you determine the
appropriate bounds.
Consider the region $D$ in space that is inside both the sphere
$x^2+y^2+z^2=9$ and the cylinder $x^2+y^2=4$. Start by drawing
the region.
- Set up an iterated integral in Cartesian (rectangular)
coordinates that would give the volume of $D$.
- Set up an iterated integral in cylindrical coordinates
that would give the volume of $D$.
Consider the region $D$ in space that is both inside the sphere
$x^2+y^2+z^2=9$ and yet outside the cylinder $x^2+y^2=4$. Start
by drawing the region.
- Set up two iterated integrals in cylindrical coordinates
that would give the volume of $D$. For one integral use the
order $dzdrd\theta$. For the other, use the order $d\theta dr
dz$.
- Set up an iterated integral in spherical coordinates that
would give the volume of $D$.
The integral
$\ds\int_{0}^{\pi}\int_{0}^{1}\int_{\sqrt{3}r}^{\sqrt{4-r^2}}rdzdrd\theta$
represents the volume of solid domain $D$ in space. Set up
integrals in both rectangular coordinates and spherical
coordinates that would give the volume of the exact same
region.
The temperature at each point in space of a solid occupying the
region {$D$}, which is the upper portion of the ball of radius
4 centered at the origin, is given by $T(x,y,z) = \sin(xy+z)$.
Set up an iterated integral formula that would give the average
temperature.
The Divergence Theorem
In definition TODO on page
\pageref{definition of flux density in 2D}, we defined the
divergence, or flux density, of a vector field $\vec F$ at a
point $P$ to be the flux per unit area, and then stated that
$\text{div}(\vec F)=M_x+N_y$. We now extend this to 3D. In 3D,
the flux of $\vec F$ across $S$, $\iint_S\vec F\cdot \vec n
d\sigma$, is a measure of flow across $S$ where $\vec n$ is a
continuous unit normal vector to $S$. Flux density at $(x,y,z)$
is found by creating a sphere $S_a$ of radius $a$ centered at
$(x,y,z)$ with interior volume $V_a$ and outward normal vector
$\vec n$, and considering the quotient of flux per volume given
by $\frac{1}{V_a}\iint_{S_a} \vec F \cdot \vec n d\sigma$. By
computing $\ds \lim_{a\to 0}\frac{1}{V_a}\iint_{S_a} \vec F \cdot
\vec n d\sigma$, we obtain the divergence of $\vec F$ at
$(x,y,z)$, also called the flux density. In a future mathematics
course, we could prove that the divergence equals \begin{align*}
\text{div}\vec F(x,y,z) &= \vec \nabla\cdot \vec F =
\left(\frac{\partial }{\partial x},\frac{\partial }{\partial
y},\frac{\partial }{\partial z} \right)\cdot (M,N,P) \\ &=
\frac{\partial M}{\partial x}+\frac{\partial N}{\partial
y}+\frac{\partial P}{\partial z} = M_x+N_y+P_z . \end{align*}
I tried problems like this during the semester in the double
integral section, and they didn't go very well. Perhaps it was
placement. It was a waste of 20 minutes in the previous
section.
As an example, we compute the flux density at $(0,0,0)$ for
the vector field $\vec F = \left<x,y,z\right>$. A
sphere of radius $a$ has unit normal vector $\vec n =
\frac{\left<x,y,z\right>}{|\left<x,y,z\right>|}$,
so the flux is $\iint_S \left<x,y,z\right>\cdot
\frac{\left<x,y,z\right>}{|\left<x,y,z\right>|}d\sigma
= \iint_S \sqrt{x^2+y^2+z^2}d\sigma = a \iint_S d\sigma =
a4\pi a^2$, since the surface area of a sphere is $4\pi a^2$.
The volume inside a sphere of radius $a$ is $\frac 43\pi
a^3$. Hence $\lim_{a\to 0}\frac{3}{4\pi a^3}4\pi a^3 = 3$,
which equals $\text{div}\vec F = M_x+N_y+P_z = 1+1+1=3$.
Let $S$ be a closed surface whose interior is the solid domain
$D$. Let $\vec n$ be an outward pointing unit normal vector to
$S$. Suppose that $\vec F(x,y,z)$ is a continuously
differentiable vector field on some open region that contains
$D$. Then the outward flux of $\vec F$ across $S$ can be
computed by adding up, along the entire solid $D$, the flux per
unit volume (divergence). Symbolically, the divergence theorem
states $$\iint_S\vec F\cdot \vec n d\sigma = \iiint_D \vec
\nabla \cdot \vec F dV = \iiint_D \left(M_x+N_y+P_z\right) dV
$$ for $S$ a closed surface with interior $D$ and outward
normal $\vec n$.
Let $S$ be the surface of the wedge in the first octant bounded
by the planes $x=1$ and $\ds\frac{y}{2}+\frac{z}{3}=1$. Let
$\vec F$ be the vector field
$\left<x+3y^2,y^2-4x,2z+xy\right>$. Use the divergence
theorem to compute the outward flux of $\vec F$ across $S$.
Make sure you draw the wedge (you may find centroids and volume
help complete this problem rapidly).
Consider the vector field $\vec F =
\left<yz,-xz,3xz\right>$. Let $D$ be the solid region in
space inside the cylinder of radius 4, above the plane $z=0$,
and below the paraboloid $z=x^2+y^2$. The surface $S$ consists
of 3 portions, so computing the flux would require a rather
time consuming process of parameterizing these 3 surfaces.
Instead, use the divergence theorem to compute the outward flux
of $\vec F$ across the surface $S$.