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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 ''x''-axis. Lebesgue integration is a mathematical Theory that extends the integral to a larger class of functions; it also extends the domains on which these functions can be defined. 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 as the integral 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 ( 1875 - 1941 ). The pronunciation of his name may be approximated in English as ''leh BEG''. 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 ( 1826 - 1866 ), is a broadly successful attempt to provide such a foundation for the integral. Riemann's definition starts with the construction of a sequence of easily-calculated 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 already-solved 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 Transform s 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 easily-calculated 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 Non-measurable 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 ''b'' × ''d'' , whose area is calculated to be (''b''-''a'')(''d''-''c''). The quantity ''b''-''a'' is the length of the base of the rectangle and ''d''-''c'' 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 (non-negative) measure on a Sigma-algebra ''X'' of subsets of ''E''. For example, ''E'' can be Euclidean ''n''-space R''n'' or some Lebesgue Measurable subset of it, ''X'' will be the sigma-algebra 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 pre-image of any closed interval is in ''X'': : It can be shown that this is equivalent to requiring that the pre-image 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: : are measurable if the original sequence {''f''''k''}, where ''k'' ∈ N, consists of measurable functions. We build up an integral : for measurable complex-valued 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: : Simple functions: We extend by linearity to the Linear Span of indicator functions: : 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 ''. Even if a simple function can be written in many ways as a linear combination of indicator functions, the integral will always be the same. Non-negative functions: Let ''f'' be a non-negative 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 : 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 non-negative extended real-valued 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 : where : : Note that both ''f''+ and ''f''− are non-negative functions. Also note that |
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