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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

Descartes to Newton

than the original one. Find the G.C.D. of the two equations. This is x − 2 ; hence 2 is one of the two equal roots. Had there been no common divisor, then the original equation would not have possessed equal roots. Hudde gave a demonstration for this rule.24

Heinrich van Heuraet must be mentioned as one of the earliest

geometers who occupied themselves with success in the rectification of curves. He observed in a general way that the

two problems of quadrature and of rectification are really identical, and that the one can be reduced to the other. Thus he carried the rectification of the hyperbola back to the quadrature of the hyperbola. The semi-cubical parabola

y3=ax2 was the first curve that was ever rectified absolutely. This appears to have been accomplished independently by Van Heuraet in Holland and by William Neil (1637–1670) in England.

According to Wallis the priority belongs to Neil. Soon after, the cycloid was rectified by Wren and Fermat.

The prince of philosophers in Holland, and one of the greatest scientists of the seventeenth century, was Christian Huygens (1629–1695), a native of the Hague. Eminent as a

physicist and astronomer, as well as mathematician, he was a worthy predecessor of Sir Isaac Newton. He studied at Leyden under the younger Van Schooten. The perusal of

some of his earliest theorems led Descartes to predict his future greatness. In 1651 Huygens wrote a treatise in which he pointed out the fallacies of Gregory St. Vincent (1584–1667)

on the subject of quadratures. He himself gave a remarkably close and convenient approximation to the length of a circular arc. In 1660 and 1663 he went to Paris and to London. In 1666 he was appointed by Louis XIV. member of the French

Academy of Sciences. He was induced to remain in Paris from that time until 1681, when he returned to his native city, partly for consideration of his health and partly on account of the revocation of the Edict of Nantes.

The majority of his profound discoveries were made with aid of the ancient geometry, though at times he used the

geometry of Descartes or of Cavalieri and Fermat. Thus,

like his illustrious friend, Sir Isaac Newton, he always showed

partiality for the Greek geometry. Newton and Huygens were kindred minds, and had the greatest admiration for each other. Newton always speaks of him as the "Summus Hugenius."

To the two curves (cubical parabola and cycloid) previously

rectified he added a third,–-the cissoid. He solved the

problem of the catenary, determined the surface of the

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