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Introduction 5.1.1
The basic idea behind integration is a very simple one, namely to measure
the area between the

-axis and the graph of a function by approximating it
with a series of rectangles. When approximating the function from below, the
total surface of the rectangles increases when refining the mesh (this is called
the lower Riemann sum). When approximating the function from above, the total
surface of the rectangles decreases when refining the mesh (this is called
the upper Riemann sum). As often seems to be the case in calculus, two pictures
can say a thousand words:
200pt
 |
|
200pt
 |
| lower Riemann sums |
|
upper Riemann sums |
The natural question to ask now is if these sums converge at all and if so if they
converge to the same number which would then be the area bounded by the

-axis
and

. The answer to this question is worded in the integrability theorem:
- Integrability Theorem: Let
be a real-valued function over
such
that
is bounded and that
is continuous except at a finite number of points,
then the upper Riemann sums and the lower Riemann sums will converge to the same
number. Such a function is then called integrable.
Note that integrability is considered over the closed interval
![$ [a,b]$](img286.png)
and not over the
open interval
![$ ]a,b[$](img296.png)
to avoid problems with arbitrarily large values, like e.g.
the values of

close to 0.
It is possible to prove integrability for much ``wilder" functions, but this would lead
to a lot of unnecessary complications. Yet, there are quite a few functions that fit this ``restrictive" conditions:
- all polynomials
and
functions
- rational functions, provided
does not contain a point where
the denominator is 0. (Note that the tangent function has essentially the
same problem with
.)
- exponential functions
- logarithmic functions when the interval is fully part of the positive
half of the
-axis
It is not difficult to come up with functions that are not integrable. Again, as was
the case for sequences, functions and derivatives, there are basically two reasons
why a function could not be integrable: because the area below the function is not
finite, or because the upper and lower Riemann sum do not converge to the same number.
Definition 5.1.2
Let

be an integrable function over the interval
![$ [a,b]$](img286.png)
then the integral
of

over
![$ [a,b]$](img286.png)
is defined as follows:
 |
(5.1.3) |
In this formula,

is the width of the rectangle in a Riemann sum, namely

. The idea is that if

gets bigger,

gets smaller and
the approximation becomes more precise.

is
any choice on the width of the rectangle of a Riemann sum, more
precisely,

is any choice in the interval
![$ [(i-1)\frac{b-a}{n},i\frac{b-a}{n}]$](img492.png)
.
If you choose

so that

is the highest value for that little interval
then you get the upper Riemann sum, if

is the lowest value for that little
interval, then you get the lower Riemann sum. Any other choice is somewhere in between,
but this doesn't matter at all, because for integrable functions, any choice converges
to the same number.
Properties 5.1.3
Let

and

be integrable functions and take

on the real line.
Let

and

be real numbers. Then the following equalities hold:
- Concatenation of Intervals
 |
(5.1.4) |
- Linearity of the Integral
![$\displaystyle \int_a^b [\alpha \cdot f(x) + \beta g(x)] dx = \alpha \cdot \int_a^b f(x)dx + \beta \cdot \int_a^b g(x)dx$](img495.png) |
(5.1.5) |
- Order Preserving Property of the Integral
 |
(5.1.6) |
The proofs of these properties are quite trivial. All three boil
down to the fact that the same relations hold for limits and sums.
It is also clear that these properties hold when looking at the integral
as a measure of area.
Theorem 5.1.4 (Anti-Derivative)
Let

be an integrable function over
![$ [a,b]$](img286.png)
. Then the following relation holds
for any

in
![$ [a,b]$](img286.png)
:
 |
(5.1.7) |
Proof.
By the definition of derivative and by property
5.1.4, we have
Furthermore, note that by the definition of upper Riemann and lower Riemann sums,
![$\displaystyle (y-x) \cdot \min_{t \in [x,y]} f(t) \leq \int_x^y f(t)dt \leq (y-x) \cdot \max_{t \in [x,y]} f(t)$](img499.png) |
(5.1.9) |
If you need convincing, have a look at the following graphs:
200pt
 |
|
200pt
 |
Therefore, we have:
![$\displaystyle \min_{t \in [x,y]} f(t) \leq \frac{1}{y-x} \int_x^y f(t)dt \leq \max_{t \in [x,y]} f(t)$](img502.png) |
(5.1.10) |
If

approaches

then naturally the minimum and maximum over
![$ [x,y]$](img504.png)
approach
each other and thus:
 |
(5.1.11) |
Remark 5.1.5
Theorem (
5.1.4) is sometimes called the fundamental theorem of
calculus because it establishes a very intricate link between integration and
differentiation. Although properties (
5.1.4), (
5.1.5)
and (
5.1.6) are quite useful, without the fundamental theorem of
calculus, you would still have to calculate any given integral by writing down
the Riemann sums and taking the limit. A very cumbersome procedure to go through,
even for the simplest of integrals, while now, we can simply state:
 |
(5.1.12) |
for any constant

because
 |
(5.1.13) |
This can easily be extended as follows:
for any constant

. This equality holds for all

and

. As it is true for any chosen
boundaries, we might as well write it as
 |
(5.1.15) |
while we actually mean (
5.1.14) for any

and

. Integrals with boundaries like
(
5.1.12) are called definite integrals while integrals without, like
(
5.1.15) are called indefinite integrals.
Also note that the more pedantic among us will insist on writing
 |
(5.1.16) |
And, quite frankly, the pedantic among us are right: this relation holds for
any constant

because

and not just for

. When calculating
integrals as such, this is not that important, as long as you are very well aware
of the fact that a constant should be added. When getting into the vast realm of
differential equations, this will be of crucial importance, because the solution
of a differential equation is invariably of the form
 |
(5.1.17) |
so assuming your constants to be 0 in this case makes you throw away
virtually all your solutions.
Remark 5.1.6
Note that there are functions that are integrable, but for which the
integral is not defined. This is not a contradiction: take e.g.
 |
(5.1.18) |
There is no closed form for this function, meaning that it is not possible to
write it without integrals or infinite sums. Yet,

is clearly an
integrable function (bounded by

and continuous). You should not think that
this is a rare situation. In fact, very standard functions as

and

cannot be written without infinite sums or in an implicit way as
solutions of a differential equation.
It is also not the case that above function is a very exotic and useless one.
In fact, this function also known as ``normal distribution" or ``Gauss" function
is one of the standard cases in probability and statistics.
Next: Integration Techniques
Up: Integration Theory
Previous: Integration Theory
  Contents
Marc Corluy
2003-08-26