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

A five star textbook for college calculus

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A50

appendix G The Logarithm Defined as an Integral

Our treatment of exponential and logarithmic functions until now has relied on our intuition,

which is based on numerical and visual evidence. (See Sections 1.4, 1.5, and 3.1.)

Here we use the Fundamental Theorem of Calculus to give an alternative treatment that

provides a surer footing for these functions.

Instead of starting with b x and defining log b x as its inverse, this time we start by defining

ln x as an integral and then define the exponential function as its inverse. You should

bear in mind that we do not use any of our previous definitions and results concerning

exponential and logarithmic functions.

The Natural Logarithm

We first define ln x as an integral.

1 Definition The natural logarithmic function is the function defined by

ln x − y x

1

1

t dt x . 0

y

y= 1 t

0

1

area=ln x

x t

FIGURE 1

y

area=_ln x

y= 1 t

0

x 1

t

FIGURE 2

y

y= 1 t

A

E

D

B C

0 1 2 t

FIGURE 3

The existence of this function depends on the fact that the integral of a continuous

function always exists. If x . 1, then ln x can be interpreted geometrically as the area

under the hyperbola y − 1yt from t − 1 to t − x. (See Figure 1.) For x − 1, we have

For 0 , x , 1,

ln x − y x

ln 1 − y 1

1

1

1

t dt − 0

1

t dt − 2 y 1 x

1

t dt , 0

and so ln x is the negative of the area shown in Figure 2.

EXAMPLE 1

(a) By comparing areas, show that 1 2 , ln 2 , 3 4 .

(b) Use the Midpoint Rule with n − 10 to estimate the value of ln 2.

SOLUTION

(a) We can interpret ln 2 as the area under the curve y − 1yt from 1 to 2. From Figure

3 we see that this area is larger than the area of rectangle BCDE and smaller than

the area of trapezoid ABCD. Thus we have

1

2 ? 1 , ln 2 , 1 ? 1 2 s1 1 1 2 d

1

2 , ln 2 , 3 4

(b) If we use the Midpoint Rule with f std − 1yt, n − 10, and Dt − 0.1, we get

ln 2 − y 2 1

1 t dt < s0.1df f s1.05d 1 f s1.15d 1 ∙ ∙ ∙ 1 f s1.95dg

− s0.1dS 1

1.05 1 1

1.15 1 ∙ ∙ ∙ 1

1.95D 1 < 0.693 ■

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