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Solutions to Math 234 Homework: Vector Calculus and Line Integrals (Spring 2008), Assignments of Advanced Calculus

Solutions to homework problems from sections 13.3 to 13.5 of a math 234 course focused on vector calculus and line integrals, taken in spring 2008. The solutions include the application of partial integration, green's theorem, and the fundamental theorem of line integrals to find potential functions, line integrals, and work done by vector fields.

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Pre 2010

Uploaded on 08/18/2009

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Solutions to Homework from Sections 13.3-13.5
Math 234, Spring 2008
Section 13.3
8. ~
F(x, y) = hP(x, y), Q(x, y )i=h1+2xy + ln x, x2i. So P
∂y = 2x=∂Q
∂x , which means ~
Fis conservative.
To find the potential function, we use partial integration:
f(x, y) = ZP(x, y)dx =x+x2y+ (xln xx) + g(y) = x2y+xln x+g(y)
Differentiating with respect to y, we find:
Q(x, y) = fy(x, y) = x2+g0(y) =x2=x2+g0(y) =g0(y) = 0
So g(y) is a constant, which we can choose to be 0. Then f(x, y) = x2y+xln x.
18. ~
F(x, y, z) = hey, xey,(z+ 1)ezi,Cis parametrized by ~r(t) = ht, t2, t3i, 0 t1.
(a) We find the potential function f(x,y , z) such that ~
F=fby partial integration of the three components of ~
F:
f(x, y, z) = Zeydx =xey+g1(y , z)
f(x, y, z) = Zxeydy =xey+g2(x, z )
f(x, y, z) = Z(z+ 1)ezdz =z ez+g3(x, y)
Combining these gives f(x, y, z) = xey+zez.
(b) By the Fundamental Theorem of Line Integrals:
ZC
~
F·d~r =f(~r (1)) f(~r(0)) = f(1,1,1) f(0,0,0) = (e+e)(0 + 0) = 2e
34. (a) Consider a vector field ~
F(~r) = c~r
|~r|3. We first observe that ~
Fis a conservative vector field. Let f(x,y , z) =
c
x2+y2+z2. Then:
f(x, y, z) = hfx, fy, fzi=ch−x, y , zi
(x2+y2+z2)3/2=chx, y, zi
(x2+y2+z2)3/2=c~r
|~r|3=~
F(~r)
So we can use the Fundamental Theorem for Line Integrals to find the work done by ~
Fin moving an object from
a point P1a distance d1from the origin to a point P2a distance d2from the origin along some path C. The work
is: ZC
~
F·d~r =f(P2)f(P1) = c
d2c
d1
=c1
d11
d2
(b) The work done by the gravitational field when the Earth moves from aphelion to perihelion is (converting all
distances to meters, to match the units of the gravitational constant G):
(mMG)1
1.52 ×1011 1
1.47 ×1011 =(5.97 ×1024)(1.99 ×1030)(6.67 ×1011 )(1011)1
1.52 1
1.47
=(79.24 ×1032)(0.0224) 1.77 ×1032 N·m
(c) The work done by the electric field is:
qQ 1
1012 2
1012 = (8.985 ×109)(1.6×1019)(1)(1012)1440
pf3

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Download Solutions to Math 234 Homework: Vector Calculus and Line Integrals (Spring 2008) and more Assignments Advanced Calculus in PDF only on Docsity!

Solutions to Homework from Sections 13.3-13.

Math 234, Spring 2008

Section 13.

F (x, y) = 〈P (x, y), Q(x, y)〉 = 〈1 + 2xy + ln x, x

2 〉. So

∂P

∂y

= 2x =

∂Q

∂x

, which means

F is conservative.

To find the potential function, we use partial integration:

f (x, y) =

P (x, y) dx = x + x

2 y + (x ln x − x) + g(y) = x

2 y + x ln x + g(y)

Differentiating with respect to y, we find:

Q(x, y) = fy (x, y) = x

2

  • g

′ (y) =⇒ x

2 = x

2

  • g

′ (y) =⇒ g

′ (y) = 0

So g(y) is a constant, which we can choose to be 0. Then f (x, y) = x

2 y + x ln x.

F (x, y, z) = 〈e

y , xe

y , (z + 1)e

z 〉, C is parametrized by ~r(t) = 〈t, t

2 , t

3 〉, 0 ≤ t ≤ 1.

(a) We find the potential function f (x, y, z) such that

F = ∇f by partial integration of the three components of

F :

f (x, y, z) =

e

y dx = xe

y

  • g 1 (y, z)

f (x, y, z) =

xe

y dy = xe

y

  • g 2

(x, z)

f (x, y, z) =

(z + 1)e

z dz = ze

z

  • g 3

(x, y)

Combining these gives f (x, y, z) = xe

y

  • ze

z .

(b) By the Fundamental Theorem of Line Integrals:

C

F · d~r = f (~r(1)) − f (~r(0)) = f (1, 1 , 1) − f (0, 0 , 0) = (e + e) − (0 + 0) = 2e

  1. (a) Consider a vector field

F (~r) =

c~r

|~r|

3.^ We first observe that^

F is a conservative vector field. Let f (x, y, z) =

c √

x

2 +y

2 +z

2

. Then:

∇f (x, y, z) = 〈fx, fy , fz 〉 = −c

〈−x, −y, −z〉

(x

2

  • y

2

  • z

2 )

3 / 2

c〈x, y, z〉

(x

2

  • y

2

  • z

2 )

3 / 2

c~r

|~r|

3

F (~r)

So we can use the Fundamental Theorem for Line Integrals to find the work done by

F in moving an object from

a point P 1 a distance d 1 from the origin to a point P 2 a distance d 2 from the origin along some path C. The work

is: (^) ∫

C

F · d~r = f (P 2 ) − f (P 1 ) =

−c

d 2

−c

d 1

= c

d 1

d 2

(b) The work done by the gravitational field when the Earth moves from aphelion to perihelion is (converting all

distances to meters, to match the units of the gravitational constant G):

−(mM G)

1. 52 × 10

11

1. 47 × 10

11

= −(5. 97 × 10

24 )(1. 99 × 10

30 )(6. 67 × 10

− 11 )(

− 11 )

= −(79. 24 × 10

32 )(− 0 .0224) ≈ 1. 77 × 10

32 N · m

(c) The work done by the electric field is:

qQ

− 12

− 12

= (8. 985 × 10

9

)(− 1. 6 × 10

− 19

)(1)(− 10

12

) ≈ 1440

Section 13.

  1. We want to compute

C

xe

− 2 x dx + (x

4

  • 2x

2 y

2 )dy, where C is the boundary of the region between the circles x

2 +y

2 = 1

and x

2

  • y

2 = 4. So P (x, y) = xe

− 2 x and Q(x, y) = x

4

  • 2x

2 y

2 .

∂Q

∂x

∂P

∂y

= (4x

3

  • 4xy

2 ) − 0 = 4x

3

  • 4xy

2

So, applying Green’s Theorem (and converting to polar coordinates):

C

xe

− 2 x dx + (x

4

  • 2x

2 y

2 )dy =

D

(4x

3

  • 4xy

2 ) dA =

2 π

0

2

1

(4r

3 sin

3 θ + 4r

3 sin θ cos

2 θ) r dr dθ

2 π

0

2

1

4 r

4 sin θ(sin

2 θ + cos

2 θ) dr dθ =

2 π

0

2

1

4 r

4 sin θ dr dθ

2 π

0

sin θ dθ

2

1

4 r

4 dr

= (cos(2π) − cos(0))

2

1

4 r

4 dr

F (x, y) = 〈x, x

3

  • 3xy

2 〉, so P (x, y) = x and Q(x, y) = x

3

  • 3xy

2

. Then:

∂Q

∂x

∂P

∂y

= (3x

2

  • 3y

2 ) − 0 = 3(x

2

  • y

2 )

So: ∮

C

F · d~r =

D

3(x

2

  • y

2

) dA =

π

0

2

0

3 r

2

r dr dθ = π

2

0

3 r

3

dr =

3 π

4

− 0

4

) = 12π

  1. The coordinates of the centroid are given by:

x =

A

D

x dA and y =

A

D

y dA

Define vector fields

F 1 = 〈P 1 , Q 1 〉 = 〈 0 ,

1

2

x

2 〉 and

F 2 = 〈P 2 , Q 2 〉 = 〈−

1

2

y

2 , 0 〉. Then

∂Q 1

∂x

∂P 1

∂y

= x − 0 = x and

∂Q 2

∂x

∂P 2

∂y

= 0 − (−y) = y. So, by Green’s Theorem:

x =

A

D

x dA =

A

C

F

1

· d~r =

A

C

x

2 dy =

2 A

C

x

2 dy

y =

A

D

y dA =

A

C

F

2

· d~r =

A

C

y

2 dx = −

2 A

C

y

2 dx

Section 13.

F (x, y, z) = 〈 3 z

2 , cos y, 2 xz〉. So the curl of

F is:

∇ ×

F =

i

j

k

∂x

∂y

∂z

3 z

2 cos y 2 xz

∂y

(2xz) −

∂z

(cos y),

∂z

(3z

2 ) −

∂x

(2xz),

∂x

(cos y) −

∂y

(3z

2 )

= 〈 0 − 0 , 6 z − 2 z, 0 − 0 〉 = 〈 0 , 4 z, 0 〉 6 = 〈 0 , 0 , 0 〉

So

F is not conservative.

  1. Show that curl(f ·

F ) = f curl

F + (∇f ) ×

F. Let

F (x, y, z) = 〈P (x, y, z), Q(x, y, z), R(x, y, z)〉.

curl(f

F ) =

i

j

k

∂x

∂y

∂z

f · P f · Q f · R

∂y

(f · R) −

∂z

(f · Q),

∂z

(f · P ) −

∂x

(f · R),

∂x

(f · Q) −

∂y

(f · P )

= 〈f y

· R + f · R y

− f z

· Q − f · Q z

, f z

· P + f · P z

− f x

· R − f · R x

, f x

· Q + f · Q x

− f y

· P − f · P y

= 〈f · Ry − f · Qz , f · Pz − f · Rx, f · Qx − f · Py 〉 + 〈fy · R − fz · Q, fz · P − fx · R, fx · Q − fy · P 〉

= f · curl

F + (∇f ) ×

F