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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

Euler, Lagrange, and Laplace

established by Euler. He invented a new algorithm for continued fractions, which he employed in the solution of

the indeterminate equation ax+by=c. We now know that substantially the same solution of this equation was given 1000 years earlier, by the Hindoos. By giving the factors of the number 22n+1 when n=5, he pointed out that this expression did not always represent primes, as was supposed by Fermat. He first supplied the proof to "Fermat's theorem,"

and to a second theorem of Fermat, which states that every prime of the form 4n+1 is expressible as the sum of two squares in one and only one way. A third theorem of Fermat, that xn+yn=zn, has no integral solution for values of n greater than 2, was proved by Euler to be correct when n=3. Euler discovered four theorems which taken together make out the great law of quadratic reciprocity, a law independently

discovered by Legendre.48 Euler enunciated and proved a

well-known theorem, giving the relation between the number of vertices, faces, and edges of certain polyhedra, which, however, appears to have been known to Descartes. The powers of Euler were directed also towards the fascinating subject of the theory of probability, in which he solved some

difficult problems.

Of no little importance are Euler's labours in analytical mechanics. Says Whewell: "The person who did most to

give to analysis the generality and symmetry which are now its pride, was also the person who made mechanics analytical; I mean Euler."11 He worked out the theory of the rotation of a body around a fixed point, established the general equations of motion of a free body, and the general equation of hydrodynamics. He solved an immense number and variety of mechanical problems, which arose in his mind on all occasions. Thus, on reading Virgil's lines, "The anchor drops, the rushing keel is staid," he could not help inquiring what would be the ship's motion in such a case. About the same time as Daniel Bernoulli he published the Principle of the Conservation of

Areas and defended the principle of "least action," advanced

by Maupertius. He wrote also on tides and on sound.

Astronomy owes to Euler the method of the variation of

arbitrary constants. By it he attacked the problem of perturbations, explaining, in case of two planets, the secular variations of eccentricities, nodes, etc. He was one of the first to take up with success the theory of the moon's motion by giving approximate solutions to the "problem of three bodies."

He laid a sound basis for the calculation of tables of the moon. These researches on the moon's motion, which captured two prizes, were carried on while he was blind, with the assistance of his sons and two of his pupils.

Most of his memoirs are contained in the transactions of the Academy of Sciences at St. Petersburg, and in those of the Academy at Berlin. From 1728 to 1783 a large portion of the Petropolitan transactions were

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