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James Stewart-Calculus_ Early Transcendentals-Cengage Learning (2015)

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Section 15.6 Triple Integrals 1033

SOLUTION The solid E is shown in Figure 9. If we regard it as a type 1 region, then we

need to consider its projection D 1 onto the xy-plane, which is the parabolic region in

Figure 10. (The trace of y − x 2 1 z 2 in the plane z − 0 is the parabola y − x 2 .)

z

y

y=≈+z@

y=4

TEC Visual 15.6 illustrates how solid

regions (including the one in Figure 9)

project onto coordinate planes.

x

0

4

E

y

0

y=≈

x

FIGURE 9

R e gion of int e gratio n

FIGURE 10

Projection onto xy-plane

From y − x 2 1 z 2 we obtain z − 6sy 2 x 2 , so the lower boundary surface of E is

z − 2sy 2 x 2 and the upper surface is z − sy 2 x 2 . Therefore the description of E

as a type 1 region is

E − hsx, y, zd | 22 < x < 2, x 2 < y < 4, 2sy 2 x 2 < z < sy 2 x 2 j

and so we obtain

FIGURE 11

Projection onto xz-plane

z

≈+z@=4

0

_2 2

The most difficult step in evaluating

a triple integral is setting up an expression

for the region of integration (such

as Equation 9 in Example 2). Remem -

ber that the limits of integra tion in

the inner integral contain at most two

variables, the limits of integration in

the middle integral contain at most one

variable, and the limits of integration in

the outer integral must be constants.

x

y y sx 2 1 z 2 dV − y 2 y sy2x2

22 y4 sx 2 1 z 2 dz dy dx

x 2 2sy2x 2

E

Although this expression is correct, it is extremely difficult to evaluate. So let’s

instead consider E as a type 3 region. As such, its projection D 3 onto the xz-plane is the

disk x 2 1 z 2 < 4 shown in Figure 11.

Then the left boundary of E is the paraboloid y − x 2 1 z 2 and the right boundary is

the plane y − 4, so taking u 1 sx, zd − x 2 1 z 2 and u 2 sx, zd − 4 in Equation 11, we have

yyy sx 2 1 z 2 dV − y Fy 4

E

D3

Although this integral could be written as

sx 2 1 z

x 2 1z

dyG 2 dA − y s4 2 x 2 2 z 2 dsx 2 1 z 2 dA

2

y 2 22 ys42x2 2s42x 2 s4 2 x 2 2 z 2 d sx 2 1 z 2 dz dx

it’s easier to convert to polar coordinates in the xz-plane: x − r cos , z − r sin . This

gives

y y sx 2 1 z 2 dV − y

E

D3

D3

y s4 2 x 2 2 z 2 dsx 2 1 z 2 dA

− y 2

0

y 2

0

− 2F 4r 3

3 2 r 5

s4 2 r 2 dr r dr d − y 2

d y 2

s4r 2 2 r 4 d dr

2

5G0

− 128

15

0

0

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