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Unit 20: The Riemann Integration




          The second view is related to the limiting process. It gives rise to an integral which is the limit  Notes
          of all the values of a function in an interval. This is the integral of a function f(x) over an interval
          [a,b,]. It is called the definite integral and is denoted by

                                             b
                                              f(x)dx
                                             a
          The definite integral is a number since geometrically it corresponds an area of a region enclosed
          by the graph of a function.
          Although both the notions of integration are closely related, yet, you will see later, the definite
          integral turns out to be a mare fundamental concept. In fact, it is the starting point for some
          important generalizations like the double integrals, triple integrals, line integrals etc., which
          you may study on Advanced Calculus.
          The integral in the anti-derivative sense was given by Neyrtan. This notion was found to be
          adequate so long as the functions to be integrated were continuous. But in the early 19th century,
          Fourier brought to light the need for making integration meaningful for the functions that are
          not continuous. He came across such functions in applied problems. Cauchy formulated rigorous
          definition of the integral of a function. He essentially provided a general theory of integration
          but only for continuous functions. Cauchy's theory of Integration for continuous functions is
          sufficient for piece-wise  continuous functions as well as  for  the  functions having isolated
          discontinuities. However, it was G.B.F. Riemann [1826-1866] a  German mathematician  who
          extended Cauchy's integral to the discontinuous functions also. Riernann answered the question
          "what is the meaning of  f(x) dx?"

          The concept of definite integral was given by Riemann in the middle of the nineteenth century.
          That is why, it is called Riemann Integral. Towards the end of 19th Century, T.J. Stieltjes [1856-
          1894] of Holland, introduced a broader concept of integration replacing certain linear functions
          used in Riemann Integral by functions of more general forms. In the beginning of this century,
          the notion of the measure of a set of real numbers paved the way to the foundation of modern
          theory of Lebesgue Integral by an eminent French Mathematician H. Lebesgue [1875-1941], a
          beautiful generalisation of Riemann Integral which you may study in some advanced courses of
          Mathematics. In this unit, the Riemann Integral will be defined without bringing in the idea of
          differentiation. As you have been go through the usual connection between the Integration and
          Differentiation. Just by applying the definition, it is not always easy to test the integrability of
          a function. Therefore, condition of integrability will be derived with the help of which it becomes
          easier  to discuss  the integrability  of functions.  Then just  as in  the case of continuity  and
          derivability, we will also consider algebra of integrable functions. Finally, in this unit, second
          definition of integral as the limit of a sum will be given to you and you will be shown the
          equivalence of the two definitions.

          20.1 Riemann Integration


          The study of the integral began with the geometrical consideration of calculating areas of plane
          figures. You know that the well-known formula for computing the area of a rectangle is equal to
          the product of the length and breadth of the rectangle. The question that arises from this formula
          is that of finding the correct modification of this formula which we can apply to other plane
          figures. To do so, consider a function defined on a closed interval [a,b] of the real line, which
          assumes a constant value K  0 throughout the interval. The graph of such a function gives rise
          to a rectangular region bounded by the X-axis and the ordinates x = a, x = b as shown in the
          Figure 20.1.




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