The Definite Integral: A Comprehensive Guide with Examples and Exercises, Summaries of Calculus

Now we give the formal definition of integrals on the numerical level, as we did for limits in §1.7 and derivatives in §2.1. Definition: Given a function ...

Typology: Summaries

2022/2023

Uploaded on 02/28/2023

myboy
myboy 🇺🇸

4.4

(76)

260 documents

1 / 5

Toggle sidebar

This page cannot be seen from the preview

Don't miss anything!

bg1
Math 132 The Definite Integral Stewart §4.2
Precise definition. We have defined the integral Rb
af(x)dx as a number ap-
proximated by Riemann sums. The integral is useful because, given a velocity
function, it computes distance traveled; given a graph, it computes an area be-
tween the graph and the x-axis. More generally, given a varying rate of change,
the integral computes the total change; or given a varying linear influence, the
integral computes its cumulative effect.
The parts of the notation Rb
af(x)dx have their own names: Ris the integral
sign; ais the lower limit of integration;bis the upper limit of integration;f(x)
is the integrand; and xis the variable of integration. Note that the variable of
integration is named only for convenience, and changing it does not change the
value of the integral: Rb
af(x)dx =Rb
af(t)dt =Rb
af(r)dr.
Now we give the formal definition of integrals on the numerical level, as we did
for limits in §1.7 and derivatives in §2.1.
Definition: Given a function f(x) and numbers ab.
For each positive integer n, we divide the interval x[a, b] into
nincrements of width x=ba
n, with division points:
a<a+∆x<a+2∆x < · · · < a+nx=b,
and we choose sample points x1, . . . , xnwith xianywhere in the
ith increment: a+(i1)∆xxia+ix. Then we let:
Zb
a
f(x)dx = lim
n→∞
n
X
i=1
f(xi)∆x= lim
n→∞ f(x1)∆x+· · ·+f(xn)∆x.
The function f(x) is integrable over [a, b] whenever the above limit
exists for every possible choice of sample points xi.
Integrable functions. Most functions are integrable unless they have a vertical
asymptote. To be precise:
Theorem: Assume f(x) is continuous for all x[a, b], except possibly
at a finite list of removable or jump discontinuities (see §1.8).
Then f(x) is integrable, meaning its Riemann sums converge to a well-
defined limit L=Rb
af(x)dx for any choice of sample points.
This is proved in courses on Real Analysis.
To understand integrability better, let’s examine the non-integrable function
f(x) = 1
x2on [a, b] = [0,1]. (We arbitrarily set f(0) = 0 to make f(x) defined for
Notes by Peter Magyar [email protected]
Here we use “limit” to mean a boundary, not a value approached by approximations.
Even more formally, Rb
af(x)dx =Lmeans that for any error tolerance ε > 0, there is some
lower bound Nsuch that any Riemann sum with more than Nterms is forced close to Lwithin
an error of ε: that is, n > N forces
Pn
i=1 f(xi)∆xL
< ε.
pf3
pf4
pf5

Partial preview of the text

Download The Definite Integral: A Comprehensive Guide with Examples and Exercises and more Summaries Calculus in PDF only on Docsity!

Math 132 The Definite Integral Stewart §4.

Precise definition. We have defined the integral

∫ (^) b a f^ (x)^ dx^ as a number ap- proximated by Riemann sums. The integral is useful because, given a velocity function, it computes distance traveled; given a graph, it computes an area be- tween the graph and the x-axis. More generally, given a varying rate of change, the integral computes the total change; or given a varying linear influence, the integral computes its cumulative effect. The parts of the notation

∫ (^) b a f^ (x)^ dx^ have their own names:^

is the integral sign; a is the lower limit of integration;∗^ b is the upper limit of integration; f (x) is the integrand; and x is the variable of integration. Note that the variable of integration is named only for convenience, and changing it does not change the value of the integral:

∫ (^) b a f^ (x)^ dx^ =^

∫ (^) b a f^ (t)^ dt^ =^

∫ (^) b a f^ (r)^ dr. Now we give the formal definition of integrals on the numerical level, as we did for limits in §1.7 and derivatives in §2.1.

Definition: Given a function f (x) and numbers a ≤ b.

  • For each positive integer n, we divide the interval x ∈ [a, b] into n increments of width ∆x = b−na , with division points:

a < a+∆x < a+2∆x < · · · < a+n∆x = b,

and we choose sample points x 1 ,... , xn with xi anywhere in the ith^ increment: a+(i−1)∆x ≤ xi ≤ a+i∆x. Then we let: ∫ (^) b

a

f (x) dx = (^) nlim→∞

∑^ n

i=

f (xi)∆x = (^) nlim→∞ f (x 1 )∆x+· · ·+f (xn)∆x.

  • The function f (x) is integrable over [a, b] whenever the above limit exists for every possible choice of sample points xi.†

Integrable functions. Most functions are integrable unless they have a vertical asymptote. To be precise:

Theorem: Assume f (x) is continuous for all x ∈ [a, b], except possibly at a finite list of removable or jump discontinuities (see §1.8). Then f (x) is integrable, meaning its Riemann sums converge to a well- defined limit L =

∫ (^) b a f^ (x)^ dx^ for any choice of sample points.

This is proved in courses on Real Analysis. To understand integrability better, let’s examine the non-integrable function f (x) = (^) x^12 on [a, b] = [0, 1]. (We arbitrarily set f (0) = 0 to make f (x) defined for

Notes by Peter Magyar [email protected] ∗ (^) Here we use “limit” to mean a boundary, not a value approached by approximations. † (^) Even more formally, ∫^ b a f^ (x)^ dx^ =^ L^ means that for any error tolerance^ ε >^ 0, there is some lower bound N such that any Riemann sum with more than N terms is forced close to L within an error of ε: that is, n > N forces ∣∣∑n i=1 f^ (xi)∆x^ −^ L

∣∣ < ε.

all x ∈ [0, 1].) The function has a vertical asymptote discontinuity at x = 0, so the Theorem does not apply. If we attempt to compute

0

1 x^2 dx^ by a Riemann sum with ∆x = 1 − n^0 = (^) n^1 and sample points xi = a+i∆x = (^) ni , we get:

∑^ n i=

1 x^2 i^ ·^ ∆x^ =^

∑n i=

n^2 i^2 ·^

1 n =^

∑n i=

n · (^) i^12 = n+ n 4 + · · · > n.

Thus, as n → ∞, the Riemann sum also gets larger and larger, and does not approach a finite limit. Geometrically, this means there is an infinite area under the curve and above the interval [0, 1] on the x-axis.

Negative integrand. So far, we have considered

∫ (^) b a f^ (x)^ dx^ with positive inte- grand f (x) ≥ 0, in which case the integral is a positive number (in fact, an area). Now suppose f (x) ≤ 0: our definition of the integral still makes sense, but it gives a negative number. For example, for the constant function f (x) = −1, we have:

∫ (^3) 1 (−1)^ dx^ =^ nlim→∞

∑^ n i=

f (xi)∆x = (^) nlim→∞

∑^ n i=

(−1)( 3 − n 1 )

= (^) nlim→∞ (−^2 n )

∑n i=

1 = (^) nlim→∞ (− n^2 ) · n = − 2.

Geometrically, we think of each term f (xi) ∆x as (height)×(width) with a “negative height” f (xi) ≤ 0, and we count this as a “negative area”. For a general graph y = f (x) passing above and below the x-axis,

∫ (^) b a f^ (x)^ dx^ computes the “signed area” between the graph and the interval [a, b] on the x-axis, with regions above the x-axis counting as positive area, and regions below counting negative.

example: We could evaluate the integral

0 (2−x)^ dx^ with Riemann sums as above, but it is easier geometrically. The function f (x) = 2−x has x-intercept x = 2; it is positive for x ∈ [0, 2] and negative for x ∈ [2, 3]. Thus the integral is the area of the triangle above [0, 2], minus the area of the triangle below [2, 3]:

But (triangle area) = 12 (base)×(height), so

0 (2−x)^ dx^ =^

1 2 (2)(2)^ −^

1 2 (1)(1) =^

3

(width)×(height) = (b−a)A, and the area is contained inside a rectangle with (width)×(height) = (b−a)B.

Computing formally, A ≤ f (xi) ≤ B implies

∑n i=1 A^ ∆x^ ≤^

∑n ∑n i=1^ f^ (xi)∆x^ ≤ i=1 B^ ∆x. Hence: ∑^ n

i=

A ∆x =

∑^ n

i=

A · b−na = (b−na)A

∑n

i=

1 = (b−na )A· n = (b−a)A,

and similarly for the upper bound. Taking limits as n → ∞ gives the desired inequalities. The Domination Rule is similar. The Splitting Rule is intuitive when a ≤ b ≤ c. The interval [a, c] splits as the union of two sub-intervals, [a, b] ∪ [b, c], so the area above [a, c] is the sum of the areas above [a, b] and [b, c], i.e.

∫ (^) c a f^ (x)^ dx^ =^

∫ (^) b a f^ (x)^ dx^ +^

∫ (^) c b f^ (x)^ dx. Furthermore, because of our extended definition of integrals, the Splitting Rule is valid no matter what the relative positions of a, b, c. For example, if a ≤ c ≤ b, then [a, b] = [a, c]∪[c, b] and clearly

∫ (^) c a f^ (x)^ dx+

∫ (^) b c f^ (x)^ dx^ =^

∫ (^) b

∫ a^ f^ (x)^ dx. Moving b c to the other side, we get: ∫ (^) c

a

f (x) dx =

∫ (^) b

a

f (x) dx −

∫ (^) b

c

f (x) dx =

∫ (^) b

a

f (x) dx +

∫ (^) c

b

f (x) dx ,

so the very same Splitting Rule applies:

∫ (^) c a f^ (x)^ dx^ =^

∫ (^) b a f^ (x)^ dx^ +^

∫ (^) c b f^ (x)^ dx. Another example: if a = c, the Splitting Rule says: ∫ (^) a

a

f (x) dx =

∫ (^) b

a

f (x) dx +

∫ (^) a

b

f (x) dx,

which is true since both sides are zero.

Basic Integrals:

∫ (^) b

a

1 dx = b − a,

∫ (^) b

a

x dx = 12 b^2 − 12 a^2 ,

∫ (^) b

a

x^2 dx = 13 b^3 − 13 a^3.

Later, we will easily evaluate these integrals by the Fundamental Theorems. For now, we can prove them directly from the Basic Summations in §4.1 Part 2. For

the third and hardest formula, we take increment ∆x = b−na , sample points xi = a + i∆x, and f (xi) = (a+i∆x)^2 = a^2 + 2ai ∆x + i^2 (∆x)^2 , giving Riemann sum:

∑^ n

i=

f (xi)∆x =

∑^ n

i=

a^2 ∆x + 2ai(∆x)^2 + i^2 (∆x)^3

= a^2 ∆x

∑^ n

i=

1 + 2a(∆x)^2

∑^ n

i=

i + (∆x)^3

∑^ n

i=

i^2

= a2 (b− na )n + 2a (b−a)

2 n^2

1 2 n(n+1) +^

(b−a)^3 n^3

1 6 n(n+1)(2n+1) = a^2 (b−a) + 2a(b−a)^2 ( 12 + (^21) n ) + (b−a)^3 ( 13 + (^21) n + (^6) n^12 )

Taking the limn→∞, the terms with n in the denominator disappear, and we get:

∫ (^) b

a

x^2 dx = a^2 (b−a) + 2a(b−a)^2 ( 12 ) + (b−a)^3 ( 13 ) = 13 b^3 − 13 a^3.

Examples.

  • Evaluate the integral: (^) ∫ 7

− 2

(3t−5)^2 dt.

We use the Integral Rules to reduce the problem to Basic Integrals. Since∫ f (x)^2 dx is NOT equal to (

f (x) dx)^2 , we must expand the integrand and apply the Sum, Difference, and Constant Multiple Rules: ∫ (^7) − 2 (3t−5)

(^2) dt = ∫^7 − 2 (9t

(^2) − 30 t + 25) dt

= 9

− 2 t

(^2) dt − 30 ∫^7 − 2 t dt^ + 25^

− 2 1 dt = 9

3 )^ − 30 (^1

2 )^ + 25 (7−(−2))

Note that the variable of integration (t or x) is irrelevant.

  • Find an upper bound for: ∫ (^7)

− 2

(3x−5)^2 (1+ cos(x^2 )) dx.

That is, we do not ask for an exact value, only an overestimate. We know that 1 + cos(x^2 ) ≤ 2, so the Domination Rule gives: ∫ (^7) − 2 (3x−5)

(^2) (1+ cos(x (^2) )) dx ≤ ∫^7 − 2 (3x−5)

(^2) (2) dx = 2(603) = 1206.