Page 99 - Schaum's Outline of Theory and Problems of Advanced Calculus
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Integrals













                     INTRODUCTION OF THE DEFINITE INTEGRAL
                        The geometric problems that motivated the development of the integral calculus (determination of
                     lengths, areas, and volumes) arose in the ancient civilizations of Northern Africa. Where solutions were
                     found, they related to concrete problems such as the measurement of a quantity of grain.  Greek
                     philosophers took a more abstract approach.  In fact, Eudoxus (around 400 B.C.) and Archimedes
                     (250 B.C.) formulated ideas of integration as we know it today.
                        Integral calculus developed independently, and without an obvious connection to differential
                     calculus. The calculus became a ‘‘whole’’ in the last part of the seventeenth century when Isaac Barrow,
                     Isaac Newton, and Gottfried Wilhelm Leibniz (with help from others) discovered that the integral of a
                     function could be found by asking what was differentiated to obtain that function.
                        The following introduction of integration is the usual one. It displays the concept geometrically and
                     then defines the integral in the nineteenth-century language of limits. This form of definition establishes
                     the basis for a wide variety of applications.
                        Consider the area of the region bound by y ¼ f ðxÞ, the x-axis, and the joining vertical segments
                     (ordinates) x ¼ a and x ¼ b.  (See Fig. 5-1.)




                             y


                                                            y = f (x)












                                                                                             x
                                                                                ξ n b
                                        a ξ 1  x 1  ξ 2 x 2  ξ 3 x 3  x n  _  2  x n  _  1
                                                                        ξ n  _  1
                                                            Fig. 5-1
                                                             90
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