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Remarkable Mathematicians From Euler to von Neumann Ioan James Mathematical Institute, Oxford THE MATHEMATICAL ASSOCIATION OF AMERICA

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Page 1: Remarkable Mathematicians

RemarkableMathematiciansFrom Euler to von Neumann

Ioan JamesMathematical Institute, Oxford

THE MATHEMATICAL ASSOCIATION OF AMERICA

Page 2: Remarkable Mathematicians

published by the press syndicate of the university of cambridgeThe Pitt Building, Trumpington Street, Cambridge, United Kingdom

cambridge university pressThe Edinburgh Building, Cambridge CB2 2RU, UK40 West 20th Street, New York, NY 10011-4211, USA477 Williamstown Road, Port Melbourne, VIC 3207, AustraliaRuiz de Alarcon 13, 28014 Madrid, SpainDock House, The Waterfront, Cape Town 8001, South Africa

mathematical association of america1529 Eighteenth St NW, Washington DC 20036, USA

http://www.cambridge.orghttp://www.maa.org

c© Ioan James 2002

This book is in copyright. Subject to statutory exceptionand to the provisions of relevant collective licensing agreements,no reproduction of any part may take place withoutthe written permission of Ioan James.

First published 2002

Printed in the United Kingdom at the University Press, Cambridge

Typeface Trump Mediaeval 9.25/13.5pt. System LATEX2ε [dbd]

A catalogue record of this book is available from the British Library

ISBN 0 521 81777 3 hardbackISBN 0 521 52094 0 paperback

Page 3: Remarkable Mathematicians

Contents

Preface page xiPrologue xiii

1 From Euler to Legendre 1

Leonhard Euler (1707–1783) 1

Jean-le-Rond d’Alembert (1717–1783) 8

Joseph-Louis Lagrange (1736–1813) 14

Gaspard Monge (1746–1818) 20

Pierre-Simon Laplace (1749–1827) 28

Adrien-Marie Legendre (1752–1833) 36

2 From Fourier to Cauchy 42

Joseph Fourier (1768–1830) 42

Sophie Germain (1776–1831) 47

Carl Friedrich Gauss (1777–1855) 58

Simeon-Denis Poisson (1781–1840) 69

Jean Victor Poncelet (1788–1867) 76

Augustin Cauchy (1789–1857) 81

3 From Abel to Grassmann 91

Niels Abel (1802–1829) 91

Carl Jacobi (1804–1851) 97

Lejeune Dirichlet (1805–1859) 103

William Rowan Hamilton (1805–1865) 109

Joseph Liouville (1809–1882) 116

Hermann Grassmann (1809–1877) 123

4 From Kummer to Cayley 129

Ernst Kummer (1810–1893) 129

Evariste Galois (1811–1832) 134

J.J. Sylvester (1814–1897) 141

Karl Weierstrass (1815–1897) 150

P.L. Chebyshev (1821–1894) 159

Arthur Cayley (1821–1895) 165

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viii Contents

5 From Hermite to Sophus Lie 173Charles Hermite (1822–1901) 173Leopold Kronecker (1823–1891) 177Bernhard Riemann (1826–1866) 182Henry Smith (1826–1883) 189Richard Dedekind (1831–1916) 195Sophus Lie (1842–1899) 200

6 From Cantor to Hilbert 208Georg Cantor (1845–1918) 208Gosta Mittag-Leffler (1846–1927) 215Felix Klein (1849–1925) 219Sonya Kovalevskaya (1850–1891) 230Henri Poincare (1854–1912) 237David Hilbert (1862–1943) 246

7 From E.H. Moore to Takagi 258E.H. Moore (1862–1932) 258Jacques Hadamard (1865–1963) 263Felix Hausdorff (1868–1942) 271Elie Cartan (1869–1951) 279Emile Borel (1871–1956) 283Teiji Takagi (1875–1960) 292

8 From Hardy to Lefschetz 299G.H. Hardy (1877–1947) 299Oswald Veblen (1880–1960) 306L.E.J. Brouwer (1881–1966) 313Emmy Noether (1882–1935) 321R.L. Moore (1882–1974) 326Solomon Lefschetz (1884–1972) 333

9 From Birkhoff to Alexander 340George Birkhoff (1884–1944) 340Hermann Weyl (1885–1955) 345George Polya (1887–1985) 350Srinivasa Iyengar Ramanujan (1887–1920) 357Richard Courant (1888–1972) 362J.W. Alexander (1888–1971) 372

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Contents ix

10 From Banach to von Neumann 380Stefan Banach (1892–1945) 380Norbert Wiener (1894–1964) 386P.S. Aleksandrov (1896–1982) 392Oscar Zariski (1899–1986) 401A.N. Kolmogorov (1903–1987) 407John von Neumann (1903–1957) 412

Epilogue 417Further Reading 423Collections 426Acknowledgements 429

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1 From Euler to Legendre

Our first six remarkable mathematicians were born in the forty-six years from 1707to 1752. Four came from France, one from each of Italy and Switzerland.

Leonhard Euler (1707–1783)

In mathematics the eighteenth century was the age of Euler, but before wecome to him it is necessary to say a fewwords about that remarkable family,the Bernoullis. Originally from Antwerp, they left the Netherlands in thelate sixteenth century to escape the Spanish persecution of Protestants andsettled in Basel, where they married into the merchant class. Generationafter generation they produced remarkablemathematicians, beginning withthe brothers Jakob and Johann, who were born too early to qualify for

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inclusion here. Johann’s quarrelsome sonDaniel falls just within our period,but like Isaac Newton he was even more remarkable as a physicist than asa mathematician. In mathematics he was overshadowed by his uncle Jakoband eclipsed by his friend Euler.

Leonhard Euler was born in Basel on April 15, 1707. His forbears wereartisans, for the most part, but his father Paul Euler was a minister of theProtestant Evangelical Reformed Church. Paul Euler knew the Bernoulliswell, since he and Johann had lived at Jakob’s house when they werestudying mathematics under him. Paul Euler’s wife, Margarete Brucker,was also the daughter of a minister. The year after their son was born thefamily moved to the nearby village of Riehen, where his father was pastor.The boy Leonhard grew up with two younger sisters, AnnaMaria andMariaMagdalena. After some early education at home he was sent back to the cityto live with his maternal grandmother and attend the old-fashioned Latinschool of Basel, where no mathematics was taught. In 1720, at the age ofthirteen, he matriculated into the faculty of philosophy at the university.At that time the education offered was only mediocre. Euler mastered allthe available subjects and graduated in 1722, at the age of fifteen. In thesame year he competed, without success, for professorships in logic and inlaw.

The next year Euler transferred to the faculty of theology, in accor-dance with his father’s wishes, but in addition to divinity he began tostudy mathematics seriously. As he wrote in his autobiographical sketch:‘I soon found an opportunity to be introduced to a famous professor JohannBernoulli. True he was very busy and so refused flatly to give me privatelessons; but he gave me much more valuable advice to start reading moredifficult mathematical books on my own and to study them as diligently asI could; if I came across some obstacle or difficulty, I was given permissionto visit him freely every Saturday afternoon and he kindly explained tome everything I could not understand.’ Although Johann Bernoulli wasrecognized as one of the leading mathematicians in Europe his ordinaryteaching was at an elementary level.

Euler received his master’s degree in 1724 at the age of seventeen afterwriting a thesis comparing the natural philosophy of Descartes with that ofNewton. By this time he had got to know several of the younger membersof the Bernoulli clan, including Johann’s son Daniel, seven years his senior.Johann himself became increasingly aware that his student was a genius.When he wrote to Euler in later years the salutations show his growingrespect: in 1728 he addressed him as ‘The very learned and ingenious young

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Leonhard Euler (1707–1783) 3

man’. The next year this had become ‘The highly renowned and learnedman’, and the year after ‘The highly renowned and by far most sagaciousmathematician’ until by 1745 he was addressing him as ‘The incomparableL. Euler, the prince among mathematicians’.

Although Eulerwas a devout Calvinist he succeeded, with the supportof Johann Bernoulli, in persuading his father that his true vocation was inmathematics, not the church. During the next two years, while seekingemployment, Euler wrote his first important memoir, on the theory ofacoustics. Also he entered a prize competition sponsored by the AcademieRoyale des Sciences in Paris (hereafter usually called the Paris Academy)concerning themasting of sailing ships, and received an honorablemention.

Prize competitions were an important feature of scientific life atleast until the end of the nineteenth century. Originally they were a wayof seeking solutions to specific problems. They usually emanated fromthe royal academies, notably those in Berlin and Paris, and although theyprovided an opportunity for an unknown young researcher it was quitenormal for the well established to enter. In the case of the Paris Academy,for example, prizes were awarded for memoirs addressing specific problemsin the mathematical or physical sciences. Among the rules of procedure,each entry had to be under a pseudonym or motto, accompanied by a sealedenvelope similarly inscribed containing the name of the author, althoughthis could often be guessed by the judges. The Bernoullis, particularlyDaniel, were often successful in these competitions.

With the support of Johann Bernoulli, Euler applied for the vacantprofessorship of physics at the University of Basel, but was turned down,partly as being too young. The prospects of a position in Switzerland did notseem hopeful. However Daniel Bernoulli had recently accepted the offer ofa senior appointment at the newly established Imperial Russian Academyof Sciences in St Petersburg (hereafter usually called the St PetersburgAcademy). In 1725 he moved there with his elder brother Nicholaus, andtwo years later arranged for his young compatriot to join him. InitiallyEuler was given a junior post in the medical section of the academy, whichmeant that he had to spend a fewmonths studying anatomy and physiology,but before long he managed to get transferred to the mathematical section,and became a member of the permanent staff. Euler lodged with DanielBernoulli and often worked with him at a time when his research interestslay mainly in mechanics and physics, particularly hydrodynamics.

Euler learnt the Russian language, and soon settled in to enjoy thesocial life of the great city. Unfortunately his arrival coincided with the

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death of Catherine the First, who had tried to continue the progressivepolicies of her late husband, the formidable Tsar Peter the Great; this wasfollowed by a period of reaction and intolerance. When Daniel Bernoullireturned to Basel after six years in the Russian capital, Euler succeeded himas the premier mathematician at the academy. In the same year, feelingfinancially secure, he married Catharina Gsell, the daughter of a Swissartist then working in Russia. They lived in a comfortable house beside theRiver Neva.

During this first St Petersburg period, which lasted fourteen years,Euler wrote both elementary and advanced mathematical textbooks for usein Russian schools, and solved many practical problems put to him by theRussian government. As well as being professor of mathematics he wasalso in charge of the department of geography, where one of his dutieswas to prepare a map of the country. However he was mainly occupiedwith mathematical research. Perhaps his best-known work of this periodis his formulation of and solution to the problem of the seven bridges ofKonigsberg, which dates from 1736. This marks the beginning of the branchof mathematics known today as graph theory; Euler uses Leibniz’ term‘analysis situs’ in this connection, perhaps having heard it from one of theBernoullis. During this time he wrote a treatise Mechanica, in which heshowed thatmathematical analysis could be applied systematically toNew-tonian dynamics. In fact during this period he wrote almost ninety worksfor publication, and made notes of various important ideas to be developedlater. He entered for the annual prize offered by the Paris Academy and wasthe winner no less than twelve times, surpassing even Daniel Bernoulli’srecord. It was during this period that he became blind in the right eye; itseems probable that the cause was scrofula (glandular tuberculosis).

Unfortunately conditions in Russia again became oppressive after thedeath of the Regent Anna Leopoldovna, mother of the infant Tsar Ivan theSixth, and so, in 1741, Euler accepted an invitation from the King of Prussia,Frederick the Great, to move to the Prussian Royal Academy of Sciencesin Potsdam (hereafter usually called the Berlin Academy), which had justbeen reorganized after a period of decline. As he was still paid a pensionby the St Petersburg Academy, for all the next twenty-five years when hewas in Berlin, effectively he was working for both. At first the Queen couldextract from Euler only monosyllables in response to her enquiries. Shetaxed him with timidity and reserve, despite the cordiality of his reception:‘Why, then, will you not talk to me?’ she asked. ‘Because, Madam, I havejust come from a country where people are hanged if they talk.’ The Eulers

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Leonhard Euler (1707–1783) 5

settled down first in a house in Behrenstrasse, which is still preserved, andthen acquired an estate in Charlottenburg, just outside the city.

It was during this period that he completed his masterpiece, thememoir on the calculus of variations called, in the lingua franca,Methodusinveniendi lineas curvas maxime minimive proprietate gaudentes. Itspublication in 1744 led to his election to the Royal Society of Londonand to its Paris Academy, among other honours. In 1750 he conjectured thefamous formula relating the number of faces, edges, and vertices of a convexpolyhedron, and attempted to prove it. In a more popular vein he publishedhis celebrated Lettres a une Princesse d’Allemagne (Letters to a GermanPrincess), consisting of lessons in science for the King’s niece, the Princessof Anhalt-Dessau. These 234 letters, written in the period 1760–2, wereamong the most successful popularizations of science in the eighteenthcentury but they were much more: apart from their ostensible purpose theyprovide us with the most exhaustive and authoritative treatment of naturalphilosophy written by a leading scientist in the eighteenth century. Theywere translated from German into several languages. But these are just afew examples of his prodigious output.

Frederick the Great saw science as the servant of the state. Itsimportance for him lay in its ability to further technological progress.Above all he sought to strengthen his army and enrich his lands. Frederickhimself had little knowledge of theoretical science or mathematics, so hegauged the importance of the achievements of the Academy’s scientistsby their practical and military applicability. Yet despite the king’s limitedconception of science a great deal of theoretical scientific research wascarried out at the Academy, since the practical problems he assigned toits staff were not unduly laborious and so plenty of time remained forindependent work. ‘I can do just what I wish [in my research]’, Euler told afriend. ‘The King calls me his professor, and I think I am the happiest manin the world.’ Unfortunately this situation was not to last.

Initially it was the great French scientist Pierre Maupertuis whopresided over the Academy. Following his death in 1759, Euler took overthe management but under the direct supervision of the King, who didnot entirely trust him. In addition to various substantial administrativeresponsibilities, Euler was asked to undertake various practical tasks, in-cluding finance, ballistics, navigation, water supply, and so on. He was alsoexpected to advise the King on such matters as the purchase of scientificinstruments, the construction ofwatermills, the administration of lotteries,the improvement of canals, and even on the construction of a stone wall

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around the garden of the academy. Although mostly absent from Berlinduring the SevenYearsWar the Prussianmonarch took a close interest in theadministration of the Academy, particularly in the making of professionalappointments. Eventually this created an impasse in his relationship withEuler, who expected some degree of academic freedom. Increasingly he fellout of favour with the King, who tended to look down on him, referring tohim as ‘my cyclops’ in allusion to his loss of the sight of one eye. So in 1766,at the age of fifty-nine, Euler left Berlin, much to the King’s displeasure, andreturned to St Petersburg.

Throughout this second period in St Petersburg, which lasted untilhis death seventeen years later, the Empress Catherine the Great, herself ofGerman origin, was on the Russian throne. She provided for him generously,even lent him one of her cooks. ‘I and all others who had the good fortune tobe some time with the Russian Imperial Academy’, he wrote later, ‘cannotbut acknowledge that we owe everything which we are and possess to thefavourable conditions which we had there.’ However Euler’s return to theRussian capital was dogged by misfortune at first. His house was burntdown and he lost many of his possessions. In addition he became almosttotally blind due to an unsuccessful operation to remove a cataract in hisone good eye. Fortunately Euler was blessed with a prodigious memory.As a boy he had memorized the entire text of Virgil’s Aeneid. His ability toperform complex calculations in his head was well known, and his memoryundoubtedly helped him to cope with blindness in the latter part of his life,one of the most fruitful periods of his career.

Euler’s first wife Catharina died in 1776. Of their thirteen children,only three sons and two daughters survived beyond their early years. Eulerwas especially fond of children, often writing mathematics with a childon his lap. In 1777 he was married again to Catharina’s half-sister, SalomeAbigail Gsell. On September 18, 1783 he suffered a stroke and died at theage of seventy-six. Earlier that day he had given a mathematics lesson toone of his grandchildren, carried out some calculations on the ascent ofballoons, and held a discussion with his assistants concerning the orbit ofthe newly discovered planet Uranus.

Euler’s energies seemed inexhaustible. In pure mathematics his ma-jor fields were calculus, differential equations, analytic and differentialgeometry of curves and surfaces, number theory, infinite series, and thecalculus of variations. In applied mathematics he created analytical me-chanics. He wrote eminently readable textbooks on mechanics, algebra,mathematical analysis, analytic geometry, differential geometry, and the

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calculus of variations that were standard works for a century or more.In mathematical physics he built on the work of Daniel Bernoulli. Inhydrodynamics, for example, he discovered the fundamental differentialequations for the motion of an ideal fluid; and he applied them to theflow of blood in the human body. In the theory of heat he followed DanielBernoulli in regarding heat as an oscillation of molecules. He was one ofthe few scientists of the eighteenth century to favour the wave as opposedto the particle theory of light. He studied the propagation of sound and heobtained many results on the refraction and dispersion of light

However Euler was also remarkable for the skill with which heappliedmathematics to practical problems. For example, he investigated thebending of beams and calculated the safety load of columns. He calculatedthe perturbative effect of celestial bodies on the orbits of planets. He calcu-lated the paths of projectiles in resistingmedia. His three volumes on opticalinstruments contributed to the design of telescopes and microscopes. Hiswork on the design of ships aided navigation. He produced a theory ofthe tides. Nor were his interests confined to subjects closely related tomathematics; he wrote about chemistry, geography, cartography, and muchelse.

No othermathematician has published asmuch as Euler did.Hewrotealmost 900 papers, memoirs, books, and other works. Of these almost halfdate from the second St Petersburg period, when he was almost blind andeverything had to be dictated to assistants. It is estimated that of all thepages published on mathematics, mathematical physics, astronomy, andthe engineering sciences during the last three-quarters of the eighteenthcentury, one third were written by Euler. Some 560 titles were published,but much remained unpublished during in his lifetime. The Opera Omniahave been appearing at the rate of one large volume a year on average forthe last seventy years (the original programme of publication is now almostcomplete). But apart from his voluminous published works Euler left a massof correspondence, personal diaries, and other papers which will continueto occupy the attention of scholars for many years to come.

Euler was a simple man, not given to envy. As was said of Leibniz, hewas glad to observe the flowering in other people’s gardens of plants whoseseeds he had provided. Euler had only a few immediate disciples, and none ofthemwas a first-class scientist; yet, as said by Laplace, he was the teacher ofall the mathematicians of his time. In mathematics the eighteenth centurycan fairly be labelled the age of Euler, but his influence on the developmentof mathematical sciences was not restricted to that period. The work of

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many outstanding nineteenth-century mathematicians arose directly fromhis.

Jean-le-Rond d’Alembert (1717–1783)

In the late seventeenth and early eighteenth centuries France had no math-ematician to compare with the English Newton or the German Leibniz.However the relative mediocrity of French mathematics which markedthe later part of the reign of Louis XIV was now followed by one ofthe brightest periods in all history, at a time when neither Britain norGermany had any great mathematicians to show. D’Alembert, the first ofthe stars of French eighteenth-century mathematics, was often in disputewith Euler. Although Euler was the more powerful mathematician of thetwo he frequently exploited d’Alembert’s ideas. However mathematicswas only one of d’Alembert’s many interests. He was a leading figure inthe Enlightenment, the international movement which took on a specialcharacter in France.

Jean-le-Rond d’Alembert was born in Paris on November 17, 1717, sothat he was ten years junior to Euler. He was the natural son of Claudine-Alexandrine Guerin, Marquise de Tencin, a well-known salon hostess andnovelist of the period, and the Chevalier Louis-CamusDestouches-Canon, acavalry officer. His mother, who was a lapsed nun, abandoned her new-bornchild on the steps of the church of Saint Jean-le-Rond, in the cloisters ofthe cathedral of Notre Dame, because she was afraid of being returned toher convent. However his father traced the child, who was being fostered inPicardy, and who had been given the Christian name of the church where hehad been left. Destouches-Canon found him a home in Paris with an artisannamed Rousseau and his wife. D’Alembert lived with them until he wasforty-seven years old, and all his best scientific and literary work was doneunder their roof. Destouches-Canon also saw to the education of the boy,and when he died provided his son, who was then only nine years old, witha modest private income for the rest of his life. His mother, whose life wasanything but virtuous, had nothing to do with him. The name d’Alembertmay be a French version of the German Darenberg, but its significance isunknown.

D’Alembert attended the College de Quatre Nations (sometimescalled afterMazarin, its founder), a Jansenist school offering a curriculum inthe classics and rhetoric – and also offeringmore than the average amount ofmathematics. In a breakwith tradition themathematics lectures there weregiven in French, rather than Latin. The school possessed an excellent library,

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of which the boy took full advantage. After obtaining the baccalaureatein 1735 he turned against a religious career, in spite of the efforts of histeachers to persuade him otherwise, and for a time studied both law andmedicine before deciding on a career as a mathematician. Although he hadreceived almost no formal scientific training, it is clear that on his own hehad become familiar not only with Newton’s works but also with those ofl’Hopital and other mathematicians of his day, particularly the Bernoullis.

In 1739,when hewas twenty-two, d’Alembert sent his first communi-cation to the Paris Academy. During the next two years he sent five more,dealing with methods of integrating differential equations and with themotion of bodies in resisting media. His communications were answeredbyAlexis Clairautwho, although only four years older than d’Alembert, wasalready an Academician. After several attempts to gain election, d’Alembertwas successful in 1741.

For the next two years he worked on various problems in ratio-nal mechanics (what would nowadays be called theoretical mechanics)

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and published his Traite de dynamique (Treatise on dynamics). In thiscelebrated work he tried to formalize the new science of mechanics onNewtonian principles. In the first part of the treatise d’Alembert developedhis own three laws of motion. Like others of his day he did not simply adoptthose of Newton, which in any case were expressed in words, not symbols.He tried to show that the first two laws followed from basic ideas of spaceand time by reasoning which was mathematical rather than physical. Itwas not until he arrived at the third law that physical assumptions wereinvolved; he implicitly assumed conservation of momentum, and eschewedthe notion of force. The principle that bears his name can already be foundin the work of Daniel Bernoulli. It is more like a convenient rule for usingNewton’s laws, and does not actually follow from them logically.

In 1744 d’Alembert published a companion volume, the Traite del’equilibre et du mouvement des fluides (Treatise on the equilibriumand on the motion of fluids), treating the major problems of fluid me-chanics then current. Clairaut published a competing work in the sameyear. D’Alembert’s next work, Reflexions sur la cause generale des vents(Reflections on the general cause of the winds), although based on falseassumptions, contained the first general use of partial differential equationsin mathematical physics. This is just one of many instances where hismethods were perfected by Euler. Another was his (incorrect) theory ofvibrating strings, where we see the first appearance of a wave equationin physics. Then d’Alembert moved into celestial mechanics and this ledhim, in 1749, to publish his masterly Recherches sur la precession desequinoxes et sur la nutation de la terre (Investigations into the precessionof the equinoxes and the nutation of the poles); nutation is a wobble of theearth’s axis, due to lunar influences. During the next decade d’Alembertwrote one more major scientific work, his three-volume Recherches surdifferentes points importantes du systeme du monde (Investigations intovarious important points concerning the solar system) of 1754/6. Devotedprimarily to the motion of the moon it was written partially to guardhis claims to originality against those of Clairaut. As often happened,d’Alembert’s theory was the better one but Clairaut’s methods were ofmore practical use to astronomers.

Having reached the top from humble beginnings d’Alembert did notwant to lose his position. Once in the Academy, he had to struggle tostay ahead of his rivals. Whether by accident or inborn competitiveness,d’Alembert always seemed to be working on the same problems as othertopmathematicians – initially Clairaut, later Daniel Bernoulli and Euler. He

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was always afraid of losing priority, and fell into a cycle of hasty publicationsfollowed by controversy over the meaning and significance of his work.Although Euler was the most able, this does not mean that the others didnot make important contributions: because he was not much concernedwith questions of priority on his own account, he was somewhat lax inacknowledging the contributions of others, and this caused a great dealof resentment. D’Alembert often had good cause to be annoyed, but hesquandered his energy in fruitless arguments instead of giving his owntheories the exposition they deserved. Many of his best ideas were notunderstood until Euler took them over.

D’Alembert submitted a memoir on fluid mechanics for a prizecompetition announced by the Berlin Academy and, although his entrywas considered the best, the prize was not awarded. D’Alembert blamedthis decision on Euler. Relations between the two men, already cool, nowdeteriorated further. The memoir in question was published in 1752 as‘Essay on a new theory of the resistance of fluids’. It was in this essay thatd’Alembert expressed the differential equations of hydrodynamics in termsof a field and gave a description of the hydrodynamic paradox. Once againd’Alembert, Clairaut, Daniel Bernoulli, and Euler were all working on thesame lines. Each of the four influenced the other three.

Despite the fact that he was an excellent writer on other subjects(the best of the age, according to Voltaire), his mathematics was seldomwell presented. One of the reasons for d’Alembert’s lack of attention to theexposition of his mathematical ideas was his involvement in the broaderintellectual life of his time. In the 1740s he became one of the group ofintellectuals known as the philosophes, joining in the mounting tide ofcriticism of the social and intellectual standards of the day. In these circles,mathematics was enjoying great prestige. Following Newton’s success inexplaining the motion of the planets it was hoped that rational enquiry,on the mathematical model, would allow the proper organization of allknowledge and the proper conduct of all human affairs. The movementto reorganize knowledge and conduct along rational lines, known as theEnlightenment, was particularly strong in France, where it was seen as ameans to attack superstition in religion, reform the law, and later over-throw existing institutions. D’Alembert spent his time, much as the otherphilosophes did, working in the morning and afternoon of each day, andpassing the evening attending the salons. Of slight build, with an expressiveface, a high-pitched voice, a gift for conversation, and a talent for mimicry,he was known for his gaiety and wit; ‘it is time I was weaned’, he explained

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when he finally left his foster-home at the age of forty-seven.The Enlightenment was not all talk, however, and one of its most

solid achievements was the seventeen-volume Encyclopaedia, edited byDenis Diderot, which appeared between 1745 and 1772. D’Alembert wrotethe important introduction to this hugework and in it summed up his viewson the unity of all knowledge. It contributed greatly to the success of theEncyclopaedia, and was the main reason for his election to the AcademieFrancaise, the literary counterpart of the Academie des Sciences, in 1754.Eighteen years later he was elected secretaire perpetuelle (permanent sec-retary) of this August body; one of his duties was to write the eulogy whenany of the Academicians died. In spite of his efforts, the Academie Francaisefailed to produce anything noteworthy in the way of literature during hisperiod of office.

D’Alembert was also scientific editor of the Encyclopaedia for a timeandwrotemany of themathematical articles. He divided the subject up intothree main branches: pure, mixed, and physico-mathematics. Pure math-ematics included arithmetic and geometry; mixed mathematics embracedmechanics, geometry, optics, acoustics, pneumatics, and the art of con-jecturing or games of chance; physico-mathematics is where mathematicalcalculation is applied to experiment and seeks to deduce physical inferenceswhose certitude is close to geometric truth.

Eventually a rift developed among the Encyclopaedists between thematerialists, led by Diderot, and the more moderate faction, led by Voltaire.Diderot leaned towards biology, for which he conjectured an absurd pseudo-mathematical basis, while deploring the ‘impracticability’ of ordinarymathematics. D’Alembert sided with Voltaire and severed his ties withthe Encyclopaedia in 1758. In the 1760s intellectual fashion was movingaway frommathematics, and d’Alembert found himself with only one otherphilosophe still interested in it, the probability theorist Condorcet. Duringthe twenty years leading up to 1780, d’Alembert published a series of whathe called Opuscules mathematiques (Mathematical essays), essays on allkinds of topics, largely going over what he had written before but withimprovements.

D’Alembert seldom travelled, leaving France only once for a shortvisit in 1764 to the court of Frederick the Great. The Prussian monarch wasenamoured of most things French. He had learned French as a child andnever did master the German language. He saw the language of Louis XIVas the language of culture, and regarded German as crude. Thus it was to hisfriend Voltaire that he had turned for plans to build up the Berlin Academy

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shortly after his accession to the Prussian throne. On the recommendationof Voltaire the King tried to persuade d’Alembert to head it, but the latterdeclined the honour and recommended Euler instead. This helped to healthe rift that had grown up between the two.

Apart from scientific subjects d’Alembert also wrote about law andon religion. He went to visit Voltaire and, under the latter’s influence, pub-lished anonymously a polemical book inwhich he called for the suppressionof both the Jansenists and the Jesuits. He clashedwith the social philosopherJean-Jacques Rousseau. He wrote about music, especially on the composerRameau’s ideas concerning musical structure. While these activities havelittle to do with science, they serve to remind us of the wide spread of hisinterests.

The love of his life was Julie de Lespinasse, the cousin of Madame duDeffand, whose salon d’Alembert frequented. After a quarrel over poachingthe salon’s members, Julie set up a salon of her own, with his help. WhenJulie became ill with smallpox, d’Alembert nursed her back to health.Whenhe himself fell sick, in 1765, she persuaded him to leave his foster homeand move in with her. For the next ten years his life revolved around Julie’ssalon, and her death in 1776 came as a cruel blow. Humiliation was added tosorrow when he discovered from her letters that she had been passionatelyinvolved with other men throughout their time together.

D’Alembert spent the last seven years of his life in a small, ratherdismal, apartment in the Louvre, to which he was entitled as permanentsecretary of the Academie Francaise. He found himself unable to workon mathematics, although it was the only thing that still interested him.Lonely and bitter, he became gloomy about the future of mathematicsitself. Nevertheless, he did what he could to support and encourage youngmathematicians. The most notable achievement of his later years was tohelp launch the careers of Lagrange and Laplace, whose work in mechanicsultimately competed with much of his own. It must have given him somesatisfaction to anticipate the future successes of his gifted proteges, eventhough they effectively ended the theory of mechanics as he knew it. Whathe could not have anticipated was that a minor element of his work, theuse of complex numbers, would blossom in the next century, and enablemathematics to break out of the bounds set by eighteenth-century thought.

Jean-le-Rond d’Alembert died on October 29, 1783, at the age of sixty-five, just a few weeks after Euler. Perhaps he lived too long. Many of theother philosophes predeceased him, and those who remained alive in the1780s were no longer the vibrant young revolutionaries they once had been.

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What political success they achieved did not lead to tangible results. Butto a large degree they had, in Diderot’s phrase, changed the general wayof thinking, and perhaps had some beneficial influence on the intellectuallife of France. His collected literary works have been published, not hismathematical works.

D’Alembert was a mathematician in the tradition of Descartes, nota scientist like Euler. As he once said, mathematics owes its certaintyto the simplicity of the things with which it deals, and this was tiedup with his view of nature: however this was not just the view of apure mathematician but included a wide range of applications. He wasinterested in questions of probability, life expectancy, and so on. He wasahead of his time in thinking about limits of functions and convergenceof series, and almost alone in his day in regarding the differential as thelimit of a function, the key concept around which calculus was eventuallyrationalized. Unfortunately his concept did not seem any more clear tohis contemporaries than other schemes for explaining the nature of thedifferential. Finally, he seems to have been the first person on record tothink of regarding time as a fourth dimension, since in 1754 he wrote: ‘I saidearlier that it is impossible to conceive of more than three dimensions. Aclever acquaintance of mine believes that one might nevertheless considertimespan as a fourth dimension, and that the product of time with volumecould in certain manner be a product of four dimensions; this idea maybe contested, but it has, it seems to me, some merit, if only because ofits novelty.’ The clever acquaintance is thought to have been d’Alemberthimself.

Joseph-Louis Lagrange (1736–1813)

Joseph-Louis Lagrange is particularly known for his uncompromisinglyformal approach to analysis and mechanics. He viewed all functions aspower series and attempted to reduce all mechanics to the analysis ofsuch functions, without the use of geometry. At his death Lagrange leftexamples to follow, new problems to solve, and techniques to develop in allbranches of mathematics. Bonaparte described him as the ‘lofty pyramid’ ofthe mathematical sciences.

In the eighteenth century, Turin was the capital of Piedmont, andthe seat of the Savoyard Kings of Sardinia. Giuseppe Francesco LudovicoLagrangia was treasurer of the Government Offices in Turin. His wife,Teresa Grosso, was the daughter of a physician in the small town ofCambiano, not far from Turin, and a member of the wealthy Conti family.

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Their son, Joseph-Louis, was born there on January 25, 1736, one of elevenchildren, most of whom did not reach maturity. Despite the wealthy familybackground they were not well off, since his father had lost most of hismoney through gambling. His son eventually came to be thankful that hewas not offered the chance to become a wealthy idler, declaring that ifhe had inherited a fortune he would probably not have cast his lot withmathematics. Because his father’s family came from Touraine he regardedhimself as French rather than Italian. His works were written in Frenchand he used the names of Lagrange or La Grange rather than Lagrangia, buthe spoke French with a distinct Italian accent all his life, and his favouritepoet was Ariosto, according to d’Alembert.

Lagrange was intended by his father to become a lawyer. As a boy heraised no particular objections to this plan, but gradually decided he wouldprefer to study the exact sciences instead. At school he read the worksof Euclid and Archimedes, without finding them particularly interesting,but the turning point came when he accidentally came across an articleby the British astronomer and mathematician Edmund Halley arguing thesuperiority of calculus over Greek mathematics. After that he began to

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study the subject with such success that by the time he was nineteen he hadbeen appointed professor of mathematics at the Royal School of Artilleryin Turin.

In 1755 Lagrange began working on some of the isoperimetric prob-lems that Euler and others were trying to solve at that time. The followingyear he applied the calculus of variations to mechanics and showed that, inthe form of the principle of least action, it offered a general procedure forsolving dynamical problems. He communicated these results to Euler whowas greatly impressed, and withheld from publication a paper of his ownwhich covered some of the same ground but used inferior methods. Thiswas at the time when Euler was director of the mathematics division of theBerlin Academy. After Lagrangewas elected associate foreignmember of theAcademy, on Euler’s nomination, he considered the possibility of movingto Berlin, but decided to stay on in Turin for the time being. With some ofhis best students he organized a society for scientific research which soondeveloped into the Royal Academy of Sciences of Turin.

In 1759 the Turin Academy published its first volume of memoirs,to which Lagrange contributed three important papers. One was on thecalculus of variations, another on the application of differential calculus tothe theory of probability, the third provided a mathematical description ofthe vibrating string which settled in favour of Euler a controversy betweend’Alembert and Euler. It demonstrated that Lagrange had carefully studiedthe works of Newton and others which have a bearing on this problem.Lagrange also contributed to later volumes of the memoirs, and in one ofhis papers we find, for the first time, the notion of eigenvalue for lineartransformations.

Throughout eighteenth-century Europe, the scientific academies en-couraged research into celestial mechanics, often offering prizes for thesolution of specific problems. The main reason was that this kind ofscience was particularly useful for navigation. In 1764 Lagrange entered acompetition sponsored by the Paris Academy to determine the gravitationalforces that caused the moon to present a relatively unchanging face to theearth, and received the Grand prize. Two years later he again won the Grandprize, this time for a partial solution to a more complicated gravitationalproblem involving the planet Jupiter, its four then-known satellites, andthe sun.

In 1763 Lagrange visited Paris; until then he had hardly gone faroutside his native city. He was received with honour; unfortunately hebecame seriously ill during his stay. D’Alembert, who had been taking an

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interest in his career, believed that Lagrange was insufficiently appreciatedin Turin. He used his influence with the result that the King of Sardiniaand his ministers made fine promises but, when nothing came of them,d’Alembert turned towards Berlin and before long Lagrange received anattractive offer from Frederick theGreat, expressing thewish of the ‘greatestking in Europe’ to have ‘the greatest mathematician in Europe’ resident athis court. Euler, as we know, was going back to St Petersburg. He offeredLagrange the opportunity to join him there, but Lagrange declined, andin 1766 became director of mathematical physics at the Berlin Academyinstead. Before leaving for the Prussian capital he made another visit toParis but again fell ill after a banquet in his honour and left without regret.

The next year Lagrange married a cousin, Vittoria Conti. In reply toan enquiry from his friend d’Alembert he wrote: ‘I don’t know whether Icalculated ill or well, or rather, I don’t believe I calculated at all; for I mighthave done as Leibniz did, who, compelled to reflect, could never make uphis mind. I confess to you that I never had a taste for marriage . . . butcircumstances decided me to engage one of my young kinswomen to takecare of me and all my affairs. If I neglected to inform you it was becausethe whole thing seemed to me so inconsequential in itself that it was notworth the trouble of informing you of it.’ However the marital relationshipdeepened over the years, and when his wife Vittoria died sixteen years laterafter a lingering illness Lagrange was heartbroken.

For mathematical research the Berlin years were fruitful. Lagrangewas not required to lecture, but he was composing memoirs nearly everymonth on subjects ranging from probability to the theory of equations. In1767 he published an important memoir ‘On the solution of numericalequations’; four years later presented another entitled ‘Reflections on thealgebraic resolution of equations’ to the Berlin Academy, where the pointof view anticipates that of Galois. In number theory Lagrange solved someof the problems posed by Fermat, including the famous theorem that everypositive integer is the sum of the squares of four integers. He continuedhis investigation of gravitational interactions between planetary bodies,winning, in 1772, his third Grand prize from the Paris Academy for amemoir on attractions between the sun, moon, and earth. In 1774 andin 1778 he again won Grand prizes, bringing his total up to four, the first forwork related to lunar movement, the second for a study of the perturbationsof comets.

During his twenty years at the Berlin Academy, Lagrange workedon what he called Mechanique Analitique (Analytical Mechanics), the

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application of calculus to the motion of rigid bodies. His conclusions wereorganized into a volume under that title published in 1788. To quote fromthe preface:

We already have various treatises on mechanics but the plan of thisone is entirely new. I have set myself the problem of reducing thisscience [mechanics], and the art of solving the problems pertaining toit, to general formulae whose simple development gives all theequations necessary for the solutions of each problem . . . No diagramswill be found in this work. The methods which I expound in itdemand neither constructions nor geometrical or mechanicalreasonings, but solely algebraic [analytic] operations subjected to auniform and regular procedure. Those who like analysis will bepleased to see mechanics become a new branch of it, and will beobliged to me for having extended its domain.

The Mechanique Analitique was his masterpiece, a scientific poemaccording to Hamilton. About 1774 there was talk of returning to Italy,possibly to Turin, or to Naples, where he might have become director of thenewly established Academy, but nothing came of it. Around 1780 Lagrangedeveloped depression and lost interest in mathematics generally for someyears. ‘I begin to feel the pull of my inertia increasing little by little, andI cannot say I shall still be doing mathematics ten years from now’, hewrote to d’Alembert, ‘it also seems to me that the mine is already too deep,and that unless new veins are discovered it will have to be abandoned.’D’Alembert, thirteen years his senior, wrote back, ‘In God’s name do notrenounce work, for you the strongest of all distractions. Good-bye, perhapsfor the last time. Keep some memory of the man who of all in the worldcherishes and honours you the most.’

Following the death of Frederick the Great in 1786 an indifferencetowards science and a resentment of foreigners arose in Berlin; meanwhilethe Italian princes redoubled their efforts to attract Lagrange to theircourts. However it was an offer from Paris which finally persuaded himto leave Berlin, after twenty very successful years. In July 1787 he became apensionnaire veteran of the Paris Academy, of which he had been a foreignassociate member since 1772. In the French capital he was received withevery mark of distinction; apartments in the Louvre were set aside forhis reception. He was always welcome at social and scientific gatherings.However his depression worsened; he was known to gaze out of the windowfor long periods of time. He told his friends and colleagues thatmathematics

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was no longer important to him.In 1792, at the age of fifty-six, Lagrange took as his second wife

Renee-Francoise-Adelaide Le Monnier, the teenage daughter of a friend andcolleague of his. His new bride was devoted to him, and it is said she helpedLagrange gradually regain his interest in mathematics and life generally.However the second marriage was childless like the first.

During the revolutionary period Lagrange managed to remain po-litically neutral, although he was granted a pension by the revolutionarygovernment and served on the Commission charged with the establishmentof standards for weights and measures, out of which the metric systememerged. We shall learn more about this commission in the profile ofLaplace. In 1793 laws came into effect which meant the arrest of allforeigners born in enemy countries and the confiscation of their property;but Lagrange was specifically exempted. The academies were suppressed,as we shall learn in the next profile, but as new institutions succeededthem positions were always found for Lagrange, whatever the governmentin power. In 1795 he was appointed professor of mathematics at the newEcole Normale, and after that closed he became professor at the EcolePolytechnique. He wrote two textbooks on calculus for students, tryingto organize and systematize what was still a difficult and incoherent set ofmethods.

Lagrange was known for his gentle demeanour and his diplomaticskills. In appearance he was of medium height, and of slight build, withpale blue eyes and a colourless complexion. In character he was nervousand timid, detested controversy and to avoid it allowed others to take thecredit for what he himself had done. At the Berlin Academy, he remainedin favour with the King, unlike Euler. When he first settled in Paris he wasdoted on by Queen Marie-Antoinette, yet later he managed to remain ongood terms with leaders of the French Revolution and later still to findfavour with Bonaparte, who consulted him frequently. He was appointedSenator, a count of the Empire, and Grand Officer of the Legion of Honour.In his seventies he began revising and extending his masterpiece, theMechanique Analitique, for a second edition. However the long hours ofwork diminished his strength and energy and he suffered increasingly fromfainting spells. He died on April 11, 1813, at the age of seventy-seven. Hisbodywas brought to rest in the Pantheon, in recognition of his contributionsto science.

Lagrange kept himself well informed about the works of other mathe-maticians. His close friendship with d’Alembert, with whom he frequently

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exchanged letters, should not obscure the striking divergence of their ideas.D’Alembert’s mathematical production was characterized by a realismwhich links him to Newton and Cauchy. Lagrange, on the other hand,displayed in his youth, and sometimes in his later years, a poetic sense thatrecalls the creative audacity of Leibniz.

Laplace, as we shall see later, was a complete contrast to Lagrangein many respects, and one has the distinct impression that Lagrange didnot care for him. In reply to a rather pompous letter from Laplace aboutthe importance of his own work, Lagrange wrote: ‘I have always regardedmathematics as an object of amusement rather than of ambition, and I canassure you that I enjoy the works of others much more than my own, withwhich I am always dissatisfied. You will see by that, if you are exempt fromjealousy by your own success, I am none the less so by my disposition.’The story is told of how one day, after Laplace had invited Lagrange todinner, Lagrange asked, ‘will it be necessary to wear the costume of asenator?’, in a mocking tone, of which everyone except Laplace sensed themalice. Although Lagrange was always reserved towards Euler, whom henever met, it was Euler, among the older mathematicians, who influencedhim most. That is why any study of his work must be preceded by oraccompanied by an examination of the work of Euler. Yet even in the faceof this great model he preserved an originality that allowed him to criticize,but above all to generalize, to systematize, and to deepen, the work of hispredecessors.

Gaspard Monge (1746–1818)

The educational reforms that began during the French Revolution had aprofound effect on the future development of science in France. GaspardMonge played a leading role in this movement, especially in the creation ofthe Ecole Polytechnique, the illustrious foundation later to inspire the SwissFederal TechnischeHochschule, theMassachusetts Institute of Technology,and other great institutions. He also helped to devise the metric system,which has spread throughout the world. The descriptive geometry whichhe largely created remains of practical importance. In pure mathematics hemay be regarded as the father of differential geometry.

Jacques Monge was a small trader operating in Beaune, the centreof the wine-producing Cote d’Or region of Burgundy. Although his wifeJeanne (nee Rousseau) was a native Burgundian, he originally came fromthe Savoy. Their eldest son Gaspard was born on May 9, 1746. In spite oftheir modest circumstances the couple made exceptional efforts to ensure