70. Estimate the numerical value of by writing it as
the sum of and . Approximate the first inte-
gral by using Simpson’s Rule with and show that the
second integral is smaller than , which is less than
0.0000001.
71. If is continuous for , the Laplace transform of is
the function defined by
and the domain of is the set consisting of all numbers for
which the integral converges. Find the Laplace transforms of
the following functions.
(a) (b) (c)
72. Show that if for , where and are
constants, then the Laplace transform exists for .
73. Suppose that and for ,
where is continuous. If the Laplace transform of is
and the Laplace transform of is , show that
74. If is convergent and and are real numbers,
show that
75. Show that .
76. Show that by interpreting the
integrals as areas.
77. Find the value of the constant for which the integral
converges. Evaluate the integral for this value of .
78. Find the value of the constant for which the integral
converges. Evaluate the integral for this value of .
79. Suppose is continuous on and . Is it
possible that is convergent?
80. Show that if and , then the following inte-
gral is convergent.
y
%
0
x
a
1 ! x
b
dx
b ( a ! 1a ( "1
x
%
0
f #x$ dx
lim
x
l
%
f #x$ ! 1!0, %$f
C
y
%
0
(
x
x
2
! 1
"
C
3x ! 1
)
dx
C
C
y
%
0
(
1
s
x
2
! 4
"
C
x ! 2
)
dx
C
x
%
0
e
"x
2
dx ! x
1
0
s
"ln y
dy
x
%
0
x
2
e
"x
2
dx !
1
2
x
%
0
e
"x
2
dx
y
a
"%
f #x$ dx !
y
%
a
f #x$ dx !
y
b
"%
f #x$ dx !
y
%
b
f #x$ dx
ba
x
%
"%
f #x$ dx
s ( aG#s$ ! sF#s$ " f #0$
G#s$f *#t$F#s$
f #t$f *
t $ 00 ' f *#t$ ' Ke
at
0 ' f #t$ ' Me
at
s ( aF#s$
aMt $ 00 ' f #t$ ' Me
at
f #t$ ! tf #t$ ! e
t
f #t$ ! 1
sF
F#s$ !
y
%
0
f #t$e
"st
dt
F
ft $ 0f #t$
x
%
4
e
"4x
dx
n ! 8
x
%
4
e
"x
2
dxx
4
0
e
"x
2
dx
x
%
0
e
"x
2
dx
63. We know from Example 1 that the region
has infinite area. Show
that by rotating about the -axis we obtain a solid with
finite volume.
64. Use the information and data in Exercises 29 and 30 of Sec-
tion 6.4 to find the work required to propel a 1000-kg satellite
out of the earth’s gravitational field.
65. Find the escape velocity that is needed to propel a rocket
of mass out of the gravitational field of a planet with mass
and radius . Use Newton’s Law of Gravitation (see Exer-
cise 29 in Section 6.4) and the fact that the initial kinetic
energy of supplies the needed work.
66. Astronomers use a technique called stellar stereography to
determine the density of stars in a star cluster from the
observed (two-dimensional) density that can be analyzed
from a photograph. Suppose that in a spherical cluster of
radius the density of stars depends only on the distance
from the center of the cluster. If the perceived star density is
given by , where is the observed planar distance from
the center of the cluster, and is the actual density, it can
be shown that
If the actual density of stars in a cluster is ,
find the perceived density .
67. A manufacturer of lightbulbs wants to produce bulbs that last
about 700 hours but, of course, some bulbs burn out faster
than others. Let be the fraction of the company’s bulbs
that burn out before hours, so always lies between 0
and 1.
(a) Make a rough sketch of what you think the graph of
might look like.
(b) What is the meaning of the derivative ?
(c) What is the value of ? Why?
68. As we saw in Section 7.5, a radioactive substance decays
exponentially: The mass at time is , where
is the initial mass and is a negative constant. The mean
life of an atom in the substance is
For the radioactive carbon isotope, , used in radiocarbon
dating, the value of is . Find the mean life of a
atom.
Determine how large the number has to be so that
y
%
a
1
x
2
! 1
dx
#
0.001
a
69.
14
C
"0.000121k
14
C
M ! "k
y
%
0
te
kt
dt
M
km#0$
m#t$ ! m#0$e
kt
t
x
%
0
r#t$ dt
r#t$ ! F*#t$
F
F#t$t
F#t$
y#s$
x#r$ !
1
2
#R " r$
2
y#s$ !
y
R
s
2r
s
r
2
" s
2
x#r$ dr
x#r$
sy#s$
rR
1
2
mv
2
0
RM
m
v
0
x!
! ! *#x, y$
&
x $ 1, 0 ' y ' 1%x+
SECTION 8.8 IMPROPER INTEGRALS
|| ||
553