Lebesgue integration

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In mathematics, the integral of a function can be regarded in the simplest case as the area between the graph of that function and the xaxis. Lebesgue integration is a mathematical theory that defines the integral for a very large class of functions. It had long been understood that for functions with a smooth enough graph (such as continuous functions on closed bounded intervals) the area under the curve could be defined and computed using techniques of approximation of the region by polygons. However, as the need to consider more irregular functions arose (for example, as a result of the limiting processes of mathematical analysis and the mathematical theory of probability) it became clear that more careful approximation techniques would be needed in order to define a suitable integral.
The Lebesgue integral plays an important role in the branch of mathematics called real analysis and in many other fields in the mathematical sciences.
The Lebesgue integral is named for Henri Lebesgue (18751941). The pronunciation of his name may be approximated as leh BEG.
Contents 
Introduction
The integral of a function f between limits a and b can be interpreted as the area under the graph of f. This is easy to understand for familiar functions such as polynomials, but what does it mean for more exotic functions? In general, what is the class of functions for which "area under the curve" makes sense? The answer to this question has great theoretical and practical importance.
As part of a general movement toward rigour in mathematics in the nineteenth century, attempts were made to put the integral calculus on a firm foundation. The Riemann integral, proposed by Bernhard Riemann (18261866), is a broadly successful attempt to provide such a foundation for the integral. Riemann's definition starts with the construction of a sequence of easilycalculated integrals which converge to the integral of a given function. This definition is successful in the sense that it gives the expected answer for many alreadysolved problems, and gives useful results for many other problems.
However, Riemann integration does not interact well with taking limits of sequences of functions, making such limiting processes difficult to analyze . This is of prime importance, for instance, in the study of Fourier series, Fourier transforms and other topics. The Lebesgue integral is better able to describe how and when it is possible to take limits under the integral sign. The Lebesgue definition considers a different class of easilycalculated integrals than the Riemann definition, which is the main reason the Lebesgue integral is better behaved. The Lebesgue definition also makes it possible to calculate integrals for a broader class of functions. For example, the Dirichlet function, which is 0 where its argument is irrational and 1 otherwise, has a Lebesgue integral, but it does not have a Riemann integral.
In the next section, we discuss the technical definition of the Lebesgue integral. Readers may skip that section and continue on to the Limitations of the Riemann integral section that follows it.
Construction of the Lebesgue integral
The discussion that follows parallels the most common expository approach to the Lebesgue integral. In this approach the theory of integration has two distinct parts:
 A theory of measurable sets and measures on these sets.
 A theory of measurable functions and integrals on these functions.
Measure theory
Measure theory initially was created to provide a detailed analysis of the notion of length of subsets of the real line and more generally area and volume of subsets of Euclidean spaces. In particular, it provided a systematic answer to the question of which subsets of R have a length. As was shown by later developments in set theory (see nonmeasurable set), it is actually impossible to assign a length to all subsets of R in a way which preserves some natural additivity and translation invariance properties. This suggests that picking out a suitable class of measurable subsets is an essential prerequisite.
Of course, the Riemann integral uses the notion of length implicitly. Indeed, the element of calculation for the Riemann integral is the rectangle [a, b] × [c, d], whose area is calculated to be (ba)(dc). The quantity ba is the length of the base of the rectangle and dc is the height of the rectangle. Riemann could only use planar rectangles to approximate the area under the curve because there was no adequate theory for measuring more general sets.
In the development of the theory in most modern textbooks (after 1950), the approach to measure and integration is axiomatic. This means that a measure is any function μ defined on certain subsets X of a set E which satisfies a certain list of properties. These properties can be shown to hold in many different cases.
The theory of measurable sets and measure (including definition and construction of such measures) is discussed in other articles. See measure.
Integration
We will work in the following abstract setup: μ is a (nonnegative) measure on a sigmaalgebra X of subsets of E. For example, E can be Euclidean nspace R^{n} or some Lebesgue measurable subset of it, X will be the sigmaalgebra of all Lebesgue measurable subsets of E, and μ will be the Lebesgue measure. In the mathematical theory of probability μ will be a probability measure on a probability space E.
In Lebesgue's theory, integrals are limited to a class of functions called measurable functions. A function f is measurable if the preimage of any closed interval is in X:
 <math> f^{1}([a,b]) \in X <math>
It can be shown that this is equivalent to requiring that the preimage of any Borel subset of R be in X. We will make this assumption from now on. The set of measurable functions are closed under algebraic operations, but more importantly the class is closed under various kinds of pointwise sequential limits:
 <math> \liminf_{k \in \mathbb{N}} f_k, \quad \limsup_{k \in \mathbb{N}} f_k <math>
are measurable if the original sequence {f_{k}}_{k ∈ N} consists of measurable functions.
We build up an integral
 <math> \int_X f d \mu \quad <math>
for measurable realvalued functions f defined on E in stages:
Indicator functions: To assign a value to the integral of the indicator function of a measurable set S consistent with the given measure μ, the only reasonable choice is to set:
 <math>\int 1_S d \mu = \mu (S)<math>
Simple functions: We extend by linearity to the linear span of indicator functions:
 <math>\int \bigg(\sum a_k 1_{S_k}\bigg) d \mu = \sum a_k \mu( S_k)<math>
where the sum is finite and the coefficients a_{k} are real numbers. Such a finite linear combination of indicator functions is called a simple function. Note that a simple function can be written in many ways as a linear combination of characteristic functions, but the integral will always be the same.
Nonnegative functions: Let f be a nonnegative measurable function on E which we allow to attain the value +∞, in other words, f takes values in the extended real number line. We define
 <math>\int_E f\,d\mu := \sup\left\{\,\int_E s\,d\mu : s\le f,\ s\ \mbox{simple}\,\right\}<math>
We need to show this integral coincides with the preceding one, defined on the set of simple functions. There is also the question of whether this corresponds in any way to a Riemann notion of integration. It is not hard to prove that the answer to both questions is yes.
We have defined the integral of f for any nonnegative extended realvalues measurable function on E. For some functions ∫f will be infinite.
Signed functions: To handle signed functions, we need a few more definitions. If f is a function of the measurable set E to the reals (including ± ∞), then we can write
 <math> f = f^+  f^, \quad <math>
where
 <math> f^+(x) = \left\{\begin{matrix} f(x) & \mbox{if} \quad f(x) \geq 0 \\ 0 & \mbox{otherwise} \end{matrix}\right. <math>
 <math> f^(x) = \left\{\begin{matrix} f(x) & \mbox{if} \quad f(x) < 0 \\ 0 & \mbox{otherwise} \end{matrix}\right. <math>
Note that both f^{+} and f^{−} are nonnegative functions. Also note that
 <math> f = f^+ + f^. \quad <math>
If
 <math> \int f d \mu < \infty, <math>
then f is called Lebesgue integrable. In this case, both integrals satisfy
 <math> \int f^+ d \mu < \infty, \quad \int f^ d \mu < \infty, <math>
and it makes sense to define
 <math> \int f d \mu = \int f^+ d \mu  \int f^ d \mu <math>
It turns out that this definition gives the desirable properties of the integral. Complex valued functions can be similarly integrated, by considering the real part and the imaginary part separately.
Intuitive interpretation
To get some intuition about the different approaches to integration, let us imagine that it is desired to find a mountain's volume (above sea level) and that the mountain's boundaries are marked out clearly (they are the boundaries of integration).
The RiemannDarboux approach: Cut the mountain up into vertical slices, each one having a square base at sealevel. Pick a pair of points inside this square, one where elevation is highest and one where elevation is lowest. Associated to these two elevations are an upper volume and lower volume obtained by multiplying the elevations by the area of the square. The upper Riemann sum is the sum of the upper volumes of all the slices, and similarly for the lower Riemann sum. The Riemann integral exists if the upper and lower Riemann sums converge as the thickness of the slices decreases to 0.
The Lebesgue approach: Draw a contour map of the mountain. For each contour (or set of contours) with the lowest height, find the total area enclosed (within the map) by this set of contours, i.e. find the "measure" of this set of contours. Multiply this measure by the height represented by the set of contours: the product will be one summand of a "Lebesgue sum".
Then find a contour, or set of contours, which are at one step higher in height (lowest height of the remaining contours). Calculate the measure of the area enclosed by them. Multiply the measure by the difference in height (from the previous step), and the product will be another summand of the "Lebesgue sum".
Repeat this process for successive higher levels of contours, until the highest set of contours has been processed. The resulting sum is the linear span: each contour corresponding to an indicator function.
The sum can be refined by adding intermediate contours to the map: halving the difference between successive heights, then recomputing the sum. The Lebesgue integral is the limit of this process.
Example
Consider the indicator function of the rational numbers, 1_{Q}. It is known 1_{Q} is nowhere continuous.
 1_{Q} is not Riemannintegrable on [0,1]: No matter how the set [0,1] is partitioned into subintervals, each partition will contain at least one rational and at least one irrational number, since rationals and irrationals are both dense in the reals. Thus the upper Darboux sums will all be one, and the lower Darboux sums will all be zero.
 1_{Q} is Lebesgueintegrable on [0,1]: Indeed it is the indicator function of the rationals so by definition
 <math> \int_{[0,1]} 1_{\mathbf{Q}} \, d \mu = \mu(\mathbf{Q} \cap [0,1]) = 0,<math>
 since Q is countable.
Limitations of the Riemann integral
Here we discuss the limitations of the Riemann integral and the greater scope offered by the Lebesgue integral. We presume a working understanding of the Riemann integral.
With the advent of Fourier series, many analytical problems involving integrals came up whose satisfactory solution required exchanging infinite summations of functions and integral signs. However, the conditions under which the integrals
 <math> \sum_k \int f_k(x) dx, \quad \int \bigg(\sum_k f_k(x) \bigg) dx <math>
are equal proved quite elusive in the Riemann framework. There are some other technical difficulties with the Riemann integral. These are linked with the limit taking difficulty discussed above.
Failure of monotone convergence. As shown above, the indicator function 1_{Q} on the rationals is not Riemann integrable. In particular, the monotone convergence theorem fails. To see why, let {a_{k}} be an enumeration of all the rational numbers in [0,1] (they are countable so this can be done.) Then let
 <math> g_k(x) = \left\{\begin{matrix} 1 & \mbox{if } x = a_k \\
0 & \mbox{otherwise} \end{matrix} \right. <math>
Then let
 <math> f_k = g_1 + g_2+ \ldots + g_k. \quad <math>
The function f_{k} is zero everywhere except on a finite set of points, hence its Riemann integral is zero. The sequence f_{k} is also clearly nonnegative and monotonously increasing to 1_{Q} is not Riemann integrable.
Unsuitability for unbounded intervals. The Riemann integral can only integrate functions on a bounded interval. The simplest extension is to define
 <math> \int_{\infty}^{+\infty} f(x) dx = \lim_{a \rightarrow \infty} \int_{a}^{+a} f(x) dx <math>
whenever the limit exists. However, this breaks the desirable property of translation invariance: if f and g are zero outside some interval [a, b] and are Riemann integrable, and if f(x) = g(x + y) for some y, then ∫ f = ∫ g. With this definition of the improper integral (this definition is sometimes called the improper Cauchy principal value about zero), the functions f(x) = (1 if x > 0, −1 otherwise) and g(x) = (1 if x > 1, −1 otherwise) are translations of one another, but their improper integrals are different.
 <math> \int f(x) dx = 0, \quad \int g(x) dx= 2 . \quad <math>
Basic theorems of the Lebesgue integral
The Lebesgue integral does not distinguish between functions which only differ on a set of μmeasure zero. To make this precise, functions f, g are said to be equal almost everywhere (or equal a.e.) iff
 <math> \mu(\{x \in E: f(x) \neq g(x)\}) = 0 <math>
 If f, g are nonnegative functions (possibly assuming the value +∞) such that f = g almost everywhere, then
 <math> \int f d \mu = \int g d \mu. <math>
 If f, g are functions such that f = g almost everywhere, then f is integrable iff g is integrable and the integrals of f and g are the same.
The Lebesgue integral has the following properties:
Linearity: If f and g are integrable functions and a and b are real numbers, then af + bg is integrable and
 <math> \int (a f + bg) d \mu = a \int f d\mu + b \int g d\mu <math>
Monotonicity: If f ≤ g, then
 <math> \int f d \mu \leq \int g d \mu. <math>
Monotone convergence theorem: Suppose {f_{k}}_{k ∈ N} is a sequence of nonnegative measurable functions such that
 <math> f_k(x) \leq f_{k+1}(x) \quad \forall k\in \mathbb{N}, \forall x \in E. <math>
Then
 <math> \lim_k \int f_k d \mu = \int \sup_k f_k d \mu. <math>
Note: The value of any one the integrals is allowed to be infinite.
Fatou's lemma: If {f_{k}}_{k ∈ N} is a sequence of nonnegative measurable functions and if f = liminf f_{k}, then
 <math> \int \liminf_k f_k d \mu \leq \liminf_k \int f_k d \mu.<math>
Again, the value of any one the integrals may be infinite.
Dominated convergence theorem: If {f_{k}}_{k ∈ N} is a sequence of measurable functions with pointwise limit f, and if there is an integrable function g such that f_{k} ≤ g for all k, then f is integrable and
 <math> \lim_k \int f_k d \mu = \int f d \mu. <math>
Proof techniques
To illustrate some of the proof techniques used in Lebesgue integration theory, we sketch a proof of the above mentioned Lebesgue monotone convergence theorem:
Let {f_{k}}_{k ∈ N} be a nondecreasing sequence of nonnegative measurable functions and put
 <math> f = \sup_{k \in \mathbb{N}} f_k <math>
By the monotonicity property of the integral, it is immediate that:
 <math> \int f d \mu \geq \lim_k \int f_k d \mu <math>
We now prove the inequality in the other direction, that is
 <math> \int f d \mu \leq \lim_k \int f_k d \mu. <math>
It follows from the definition of integral, that there is a nondecreasing sequence g_{n} of nonnegative simple functions which converges to f pointwise almost everywhere and such that
 <math> \lim_k \int g_k d \mu = \int f d \mu. <math>
Therefore, it suffices to prove that for each k ∈ N,
 <math> \int g_k d \mu \leq \lim_j \int f_j d \mu. <math>
We will show that if g is a simple function and
 <math> \lim_j f_j(x) \geq g(x) <math>
almost everywhere, then
 <math> \lim_j \int f_j d \mu \geq \int g d \mu.<math>
By breaking up the function g into its constant value parts, this reduces to the case in which g is the indicator function of a set. The result we have to prove is then
 Suppose A is a measurable set and {f_{k}}_{k ∈ N} is a nondecreasing sequence of measurable functions on E such that
 <math> \lim_n f_n (x) \geq 1 <math>
 for almost all x ∈ A. Then
 <math> \lim_n \int f_n d\mu \geq \mu(A). <math>
To prove this result, fix ε > 0 and define the sequence of measurable sets
 <math> B_n = \{x \in A: f_n(x) \geq 1  \epsilon \}. <math>
By monotonicity of the integral, it follows that for any n ∈ N,
 <math> \mu(B_n) (1  \epsilon) = \int (1  \epsilon)
1_{B_n} d \mu \leq \int f_n d \mu <math>
By assumption,
 <math> \bigcup_i B_i = A, <math>
up to a set of measure 0. Thus by countable additivity of μ
 <math> \mu(A) = \lim_n \mu(B_n) \leq \lim_n (1  \epsilon)^{1} \int f_n d
\mu. <math>
As this is true for any positive ε the result follows.
Alternative formulations
If f is nonnegative, then ∫f dμ is precisely the area under the curve as measured by the product measure μ × λ where λ is the Lebesgue measure for R.
One can try to circumvent measure theory entirely. The Riemann integral exists for any continuous function f of compact support. Then we use functional analysis to obtain the integral for more general functions. Let C_{c} be the space of all realvalued compactly supported continuous functions of R. Define a norm on C_{c} by
 <math> \f\ = \int f(x) dx <math>
Then C_{c} is a normed vector space (and in particular, it is a metric space.) All metric spaces have completions, so let L^{1} be its completion. This space is isomorphic to the space of Lebesgue integrable functions (modulo sets of measure zero). Furthermore, the Riemann integral ∫ defines a continuous functional on C_{c} which is dense in L^{1} hence ∫ has a unique extension to all of L^{1}. This integral is precisely the Lebesgue integral.
The problem with this approach is that integrable functions are represented as elements of an abstractly defined completion and showing how these abstractly defined elements are represented as functions is nontrivial. In particular, the relation between pointwise limits of sequence of functions and the integral is hard to prove.
Another approach is offered by the Daniell integral or the Bourbaki variant of the Daniell integral, often referred to as the Radon measure approach to integration.
Quote
 "Does anyone believe that the difference between the Lebesgue and Riemann integrals can have physical significance, and that whether say, an airplane would or would not fly could depend on this difference? If such were claimed, I should not care to fly in that plane." Richard Hamming
See also
References
 R. M. Dudley, Real Analysis and Probability, Wadsworth & Brookes/Cole, 1989. Very thorough treatment, particularly for probabilists with good notes and historical references.
 P. R. Halmos, Measure Theory, D. van Nostrand Company, Inc. 1950. A classic, though somewhat dated presentation.
 L. H. Loomis, An Introduction to Abstract Harmonic Analysis, D. van Nostrand Company, Inc. 1953. Includes a presentation of the Daniell integral.
 H. Lebesgue, Oeuvres Scientifiques, L'Enseignement Mathématique, 1972
 M. E. Munroe, Introduction to Measure and Integration, Addison Wesley, 1953. Good treatment of the theory of outer measures.
 W. Rudin, Principles of Mathematical Analysis Third edition, McGraw Hill, 1976. Known as Little Rudin, contains the basics of the Lebesgue theory, but does not treat material such as Fubini's theorem.
 W. Rudin, Real and Complex Analysis, McGraw Hill, 1966. Known as Big Rudin. A complete and careful presentation of the theory. Good presentation of the Riesz extension theorems. However, there is a minor flaw (in the first edition) in the proof of one of the extension theorems. The discovery of which constitutes exercise 21 of Chapter 2.de:LebesgueIntegral
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