The Chemistry Maths Book, Second Edition

(Grace) #1

5.2 The indefinite integral 127


It is readily verified that this distance is equal to the area, shaded in the figure, bounded


by the linev(t)and the t-axis betweent


A

andt


B

. We shall see that this last result is valid


for any velocity functionv(t). We shall also see that the solution of a physical problem


is often equivalent to finding the area enclosed by an appropriate curve.


This example demonstrates the two central problems of seventeenth-century


European mathematics; the ‘problem of tangents’ and the ‘problem of quadrature’.


The first of these, to find the tangent lines to an arbitrary curve, led to the invention of


the differential calculus, the subject of Chapter 4. The second, to find the area enclosed


by a given curve, led to the invention of the integral calculus.


2

The demonstration by


Leibniz and by Newton that differentiation and integration are essentially inverse


operations is one of the landmarks of the history of mathematics.


The concept of integration as the inverse operation to differentiation leads to the


definition of the indefinite integral. The concept of the integral as an area leads to the


definition of the definite integral.


5.2 The indefinite integral


Lety 1 = 1 F(x)be a function of xwhose derivative is. The indefinite integral


of the derivative is defined by


Fx′ =


dy


dx


()


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Figure 5.2


2

Integration has its origins in the Greek ‘method of exhaustion’ for finding areas and volumes. Archimedes


in his Quadrature of the parabolaattributed the method to Eudoxus of Cnidus (c. 408–355 BC). In the Method,


discovered in Constantinople in 1906 after being ‘lost’ for over a thousand years, Archimedes describes how a


plane area can be regarded as a sum of line segments. In 1586, Stevin described how the centroid of a triangle can


be obtained by considering the area as made up of a large number of parallelograms. Johann Kepler (1571–1630),


best known for his Astronomia novaof 1609, computed areas and volumes by considering them to be composed


of infinitely many infinitesimal elements. His work on volumes appeared in 1615 in Nova stereometria doliorum


vinariorum(New solid geometry of wine barrels). Galileo Galilei (1564–1642) made use of the infinitely small in


his work on dynamics. Bonaventura Cavalieri (1598–1647), a follower of Galileo, described in his influential


Geometria indivisibilibus continuorum, 1635, how an area can be thought of as made up of lines or ‘indivisibles’


and a volume of areas, and developed a geometric method for finding the integral ofx


n

for positive integers n. At


about the same time, Fermat solved the same problem for positive and negative integers (exceptn 1 = 1 − 1 ) and for


fractions by dividing his areas into suitable rectangular strips. The case ofn 1 = 1 − 1 was treated by Gregoire de Saint


Vincent (1584–1667). Roberval integrated the sine function in 1635, and Torricelli the log function in 1646. Other


contributors include Pascal, whose Traité des sinus du quart de cercleof 1658 Leibniz said inspired his discovery of


the fundamental theorem, John Wallis (1616–1703), whose work on infinite processes influenced Newton and to


whom we owe the symbol ∞, the Scot James Gregory (1638–1675) whose work on infinite series and the calculus


anticipated that of Newton, and Barrow, whose lectures Newton attended and a copy of whose Lectioneswas


bought by Leibniz when on a visit to London in 1673. The final step in the synthesis of the differential and integral


calculus was taken by Newton (Footnote 3, Chapter 4) and by Leibniz, who published the first account of his


integral calculus, Analysi indivisibilium atque infinitorum(Analysis of indivisibles and infinities) in 1686.

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