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nydus/A History of MathematicsPublic

This text examines the transition from the Middle Ages to the Modern era, highlighting how the fall of Constantinople and the invention of the printing press catalyzed a revival of classical learning. It traces the shift toward scientific inquiry through the rise of pure mathematics and astronomy, detailing the intellectual struggle against established scholastic and ecclesiastical authority.

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Table of Contents

Vieta to Descartes

introduced a new idea into geometry; namely, that of infinitely great and infinitely small quantities. Greek mathematicians always shunned this notion, but with it modern mathematicians have completely revolutionised the science. In comparing rectilinear figures, the method of superposition was employed by the ancients, but in comparing rectilinear and curvilinear figures with each other, this method failed because no addition or subtraction of rectilinear figures could ever produce curvilinear ones. To meet this case, they devised the Method of Exhaustion, which was long and difficult; it was purely

synthetical, and in general required that the conclusion should be known at the outset. The new notion of infinity led

gradually to the invention of methods immeasurably more powerful. Kepler conceived the circle to be composed of an infinite number of triangles having their common vertices at the centre, and their bases in the circumference; and the sphere to consist of an infinite number of pyramids. He applied conceptions of this kind to the determination of the areas and volumes of figures generated by curves revolving about any line as axis, but succeeded in solving only a few of the simplest out of the 84 problems which he proposed for investigation in his Stereometria.

Other points of mathematical interest in Kepler's works are (1) the statement of the earliest problem of inverse tangents;

(2) an investigation which amounts to the evaluation of the definite integral 0ϕsinϕdϕ=1cosϕ; (3) the assertion that the circumference of an ellipse, whose axes are 2a and 2b, is nearly π(a+b); (4) a passage from which it has been inferred that Kepler knew the variation of a function near its maximum value to disappear; (5) the assumption of the principle of continuity (which differentiates modern from ancient

geometry), when he shows that a parabola has a focus at

infinity, that lines radiating from this "cæcus focus" are

parallel and have no other point at infinity.

The Stereometria led Cavalieri, an Italian Jesuit, to the

consideration of infinitely small quantities. Bonaventura Cavalieri (1598–1647), a pupil of Galileo and professor at

Bologna, is celebrated for his Geometria indivisibilibus continuorum nova quadam ratione promota, 1635. This work expounds his method of Indivisibles, which occupies an intermediate

place between the method of exhaustion of the Greeks and the methods of Newton and Leibniz. He considers lines as composed of an infinite number of points, surfaces as composed of an infinite number of lines, and solids of an infinite number of planes. The relative magnitude of two solids or surfaces could then be found simply by the summation of series of planes or lines. For example, he finds the sum of the squares of all lines making up a triangle equal to one-third the sum of the squares of all lines of a parallelogram of equal base and altitude; for if in a triangle, the first line at the apex be 1, then the second is 2, the third is 3, and so on; and the sum of their squares is 1 2 + 2 2 + 3 2 + ⋯ + n 2 = n ( n + 1 ) ( 2 n + 1 ) ÷ 6 . In

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