It was almost a matter of course that the English should at first have adopted the notation of Newton in the infinitesimal calculus in preference to that of Leibnitz and consequently the English school would in any case have developed on somewhat different lines to that on the continent, where a knowledge of the infinitesimal calculus was derived solely from Leibnitz and the Bernoullis. But this separation into two distinct schools became very marked owing to the action of Leibnitz and John Bernoulli, which was naturally resented by Newton's friends; and so for forty or fifty years, to the disadvantage of both sides, the quarrel raged. The leading members of the English school were Cotes, Demoivre, Ditton, David Gregory, Halley, Maclaurin, Simpson, and Taylor. I may, however, again remind my readers that as we approach modern times the number of capable mathematicians in Britain, France, Germany and Italy becomes very considerable, but that in a popular sketch like this book it is only the leading men whom I propose to mention.
To David Gregory, Halley and Ditton I need devote but few words.
David Gregory
David Gregory, the nephew of the James Gregory mentioned above, born at Aberdeen on June 24, 1661, and died at Maidenhead on Oct. 10, 1708, was appointed professor at Edinburgh in 1684, and in 1691 was on Newton's recommendation elected Savilian professor at Oxford. His chief works are one on geometry, issued in 1684; one on optics, published in 1695, which contains [p. 98] the earliest suggestion of the possibility of making an achromatic combinations of lenses; and one on the Newtonian geometry, physics, and astronomy, issued in 1702.
Halley
Edmund Halley, born in London in 1656, and died at Greenwich in 1742, was educated at St. Paul's School, London, and Queen's College, Oxford, in 1703 succeeded Wallis as Savilian professor, and subsequently in 1720 was appointed astronomer-royal in succession to Flamsteed, whose Historia Coelestis Britannica he edited; the first and imperfect edition was issued in 1712. Halley's name will be recollected for the generous manner in which he secured the immediate publication of Newton's Principia in 1687. Most of his original work was on astronomy and allied subjects, and lies outside the limits of this book; it may be, however, said that the work is of excellent quality, and both Lalande and Mairan speak of it in the highest terms. Halley conjecturally restored the eighth and lost book of the conics of Apollonius, and in 1710 brought out a magnificent edition of the whole work; he also edited the works of Serenus, those of Menelaus, and some of the minor works of Apollonius. He was in his turn succeeded at Greenwich as astronomer-royal by Bradley.
Ditton
Humphry Ditton was born at Salisbury on May 29, 1675, and died in London in 1715 at Christ's Hospital, where he was mathematical master. He does not seem to have paid much attention to mathematics until he came to London about 1705, and his early death was a distinct loss to English science. He published in 1706 a text book on fluxions; this and another similar work by William Jones, which was issued in 1711, occupied in England much the same place as l'Hospital's treatise did in France. In 1709 Ditton issued an algebra, and in 1712 a treatise on perspective. He also wrote numerous papers in the Philosophical Transactions . He was the earliest writer to attempt to explain the phenomenon of capillarity on mathematical principles; and he invented a method for finding the longditude, which has been since used on various occasions.
Cotes
Roger Cotes was born near Leicester on July 10, 1682, and died at Cambridge on June 5, 1716. He was educated at Trinity College, Cambridge, of which society he was a fellow, and in 1706 was elected to the newly-created Plumian chair of astronomy in the university of Cambridge. From 1709 to 1713 his time was mainly occupied in editing the second edition of the Principia . The remark of Newton that if only Cotes had lived "we might have known something" indicates the opinion of his abilities held by most of his contemporaries.
Cotes's writings were collected and published in 1722 under the titles Harmonia Mensurarum and Opera Miscellanea . His lectures on hydrostatics were published in 1738. A large part of the Harmonia Mensurarum is given up to the decomposition and integration of rational algebraical expressions. That part which deals with the theory of partial fractions was left unfinished, but was completed by de Moivre. Cotes's theorem in trigonometry, which depends on forming the quadratic factors of x n - 1, is well known. The proposition that "if from a fixed point O a line be drawn cutting a curve in Q 1 , Q 2 , ... , Q n , and a point P be taken on the line so that the reciprocal of OP is the arithmetic mean of the reciprocals of OQ 1 , OQ 2 , ... , OQ n , then the locus of P will be a straight line" is also due to Cotes. The title of the book was derived from the latter theorem. The Opera Miscellanea contains a paper on the method for determining the most probable result from a number of observations. This was the earliest attempt to frame a theory of errors. It also contains essays on Newton's Methodus Differentialis , on the construction of tables by the method of differences, on the descent of a body under gravity, on the cycloidal pendulum, and on projectiles.
de Moivre
Abraham de Moivre was born at Vitry on May 26, 1667, and died in London on November 27, 1754. His parents came to England when he was a boy, and his education and friends were alike English. His interest in the higher mathematics is said to have originated in his coming by chance across a copy of Newton's Principia . From the éloge on him delivered in 1754 before the French Academy it would seem that his work as a teacher of mathematics had led him to the house of the Earl of Devonshire at the instant when Newton, who had asked permission to present a copy of his work to the earl, was coming out. Taking up the book, and charmed by the far-reaching conclusions and the apparent simplicity of the reasoning, de Moivre thought nothing would be easier than to master the subject, but to his surprise found that to follow the argument overtaxed his powers. He, however, bought a copy, and as he had but little leisure he tore out the pages in order to carry one or two of them loose in his pocket so that he could study them in the intervals of his work as a teacher. Subsequently he joined the Royal Society, and became intimately connected with Newton, Halley, and other mathematicians of the English school. The manner of his death has a certain interest for psychologists. Shortly before it he declared that it was necessary for him to sleep some ten minutes or a quarter of an hour longer each day than the preceding one. The day after he had thus reached a total of something over twenty-three hours he slept up to the limit of twenty-four hours, and then died in his sleep.
He is best known for having, together with Lambert, created that part of trigonometry which deals with imaginary quantities. Two theorems on this part of the subject are still connected with his name, namely, that which asserts that sin nx + i cos nx is one of the values of (sin x + i cos x ) n , and that which gives the various quadratic factors of x 2 n - 2 px n + 1. His chief works, other than numerous papers in the Philosophical Transactions , were The Doctrine of Chances , published in 1718, and the Miscellanea Analytica , published in 1730. In the former the theory of recurring series was first given, and the theory of partial fractions which Cotes's premature death had left unfinished was completed, while the rule for finding the probability of a compound event was enunciated. The latter book, besides the trigonometrical propositions mentioned above, contains some theorems in astronomy, but they are treated as problems in analysis.
Stewart
Maclaurin was succeeded in his chair at Edinburgh by his pupil Matthew Stewart, born at Rothesay in 1717 and died at Edinburgh on January 23, 1785, a mathematician of considerable power, to whom I allude in passing, for his theorems on the problem of three bodies, and for his discussion, treated by transversals and involution, of the properties of the circle and straight line.
Antecedentes y contexto histórico
Este texto ofrece una fascinante visión del desarrollo de las matemáticas y la astronomía en Gran Bretaña a finales del siglo XVII y principios del XVIII. Describe la rivalidad entre las escuelas inglesa y continental de cálculo, centrándose en los seguidores de Isaac Newton y Gottfried Wilhelm Leibniz. Esta rivalidad marcó el rumbo del pensamiento matemático durante décadas. Las figuras mencionadas —David Gregory, Edmund Halley, Humphry Ditton, Roger Cotes, Abraham de Moivre y Matthew Stewart— fueron contribuyentes clave al avance de la ciencia y las matemáticas durante este período.
Acerca de los autores y matemáticos
- Isaac Newton (1643–1727): Aunque no se detalla aquí, la obra de Newton sentó las bases de gran parte del cálculo y la física que se discuten. Su "Principia Mathematica" revolucionó la comprensión del movimiento y la gravedad.
- David Gregory (1661–1708): Matemático y astrónomo que contribuyó a la geometría y la óptica, incluidas las primeras ideas sobre las lentes acromáticas.
- Edmund Halley (1656–1742): Famoso por el cometa Halley, también fue fundamental para la publicación de la obra de Newton e hizo importantes contribuciones a la astronomía.
- Humphry Ditton (1675–1715): Conocido por sus libros de texto sobre fluxiones (cálculo) y álgebra, y por sus primeros trabajos sobre capilaridad y cálculo de la longitud.
- Roger Cotes (1682–1716): Editor de la segunda edición de los Principia de Newton, conocido por importantes teoremas en trigonometría y los primeros trabajos sobre la teoría de errores.
- Abraham de Moivre (1667–1754): Pionero en la teoría de la probabilidad y la trigonometría que involucra números imaginarios, su trabajo sentó las bases de la estadística.
- Matthew Stewart (1717–1785): Conocido por su trabajo sobre el problema de los tres cuerpos y las propiedades geométricas.
Interpretación detallada y significado
Esta colección de biografías y logros destaca la naturaleza colaborativa y, a veces, competitiva del progreso científico. La preferencia de la escuela inglesa por la notación de Newton influyó en la dirección del cálculo en Gran Bretaña, mientras que los matemáticos continentales siguieron el enfoque de Leibniz. La disputa entre estas escuelas frenó el progreso, pero también agudizó el rigor matemático.
Las obras mencionadas, que van desde la geometría y la óptica hasta la astronomía y la probabilidad, muestran lo interconectados que estaban estos campos. Por ejemplo, los esfuerzos de Halley aseguraron que las ideas revolucionarias de Newton llegaran a un público más amplio, mientras que la teoría de la probabilidad de De Moivre se ha convertido en fundamental para la estadística y el análisis de riesgos en la actualidad.
Lecciones e ideas para los estudiantes
- Persistencia y curiosidad: Muchos de estos matemáticos se enfrentaron a desafíos, desde disputas intelectuales hasta dificultades personales. Su persistencia en el estudio de problemas complejos enseña a los estudiantes el valor de la dedicación.
- Aprendizaje interdisciplinario: La combinación de geometría, física, astronomía y probabilidad ilustra la importancia de conectar diferentes campos para resolver problemas.
- Colaboración y respeto: A pesar de las rivalidades, estos académicos a menudo se basaron en el trabajo de los demás. Esto demuestra la importancia de respetar las contribuciones de los demás y trabajar juntos.
- Innovación y pensamiento crítico: El enfoque de De Moivre sobre los números imaginarios y la probabilidad demuestra cómo el pensamiento innovador puede abrir nuevas áreas de conocimiento.
- Aplicaciones prácticas: Desde la mejora de la navegación mediante el cálculo de la longitud hasta la comprensión de la capilaridad, estos descubrimientos tuvieron impactos en el mundo real, lo que anima a los estudiantes a ver la relevancia de las matemáticas y la ciencia.
Aplicación de estas lecciones en la vida diaria
- En el aprendizaje: Emular la curiosidad y la disciplina de estos matemáticos abordando temas desafiantes paso a paso y buscando comprender sus aplicaciones en el mundo real.
- En entornos sociales: Apreciar los diversos puntos de vista y colaborar con respeto, reconociendo que el progreso a menudo proviene del esfuerzo compartido.
- En la resolución de problemas: Utilizar enfoques interdisciplinarios: combinar conocimientos de diferentes áreas para encontrar soluciones creativas.
- En el crecimiento personal: Desarrollar la paciencia y la persistencia, sabiendo que el dominio requiere tiempo y esfuerzo.
Cultivar rasgos positivos a partir de estas historias
Los estudiantes pueden aprender a valorar el aprendizaje permanente, a aceptar los desafíos y a mantener la humildad intelectual. Las historias animan a abrazar nuevas ideas, incluso cuando son difíciles, y destacan la importancia de contribuir a una comunidad de conocimiento más amplia.
Al estudiar estas figuras históricas y su trabajo, los estudiantes no solo adquieren conocimientos matemáticos, sino también la inspiración para seguir sus propios caminos en la ciencia, la tecnología, la ingeniería y las matemáticas (STEM), fomentando una mentalidad que valora la curiosidad, la colaboración y la perseverancia.
