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Leibniz–Newton calculus controversy

Public dispute between Isaac Newton and Gottfried Leibniz (beginning 1699)

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Newton began working on a form of calculus, which he called "The Method of Fluxions and Infinite Series," in 1666 at the age of 23. Although a surviving manuscript from October 1666 records this early work, it was not published until decades later in 1737 as a minor annotation in the back of one of his works. He further developed his ideas in De analysi per aequationes numero terminorum infinitas, written in 1669, and Method of Fluxions, written in 1671. Gottfried Leibniz began developing his own variant of calculus in 1674 and published his first paper on the subject, "Nova Methodus pro Maximis et Minimis," in 1684. In 1696, Guillaume de l'Hôpital published a text on Leibnizian calculus, in which he recognized that Newton's Principia of 1687 was "nearly all about this calculus." Meanwhile, Newton had presented a geometrical form of calculus in Section I of Book I of the Principia of 1687, but did not publish his eventual fluxional notation for the calculus in print until 1693 in partial form and 1704 more fully.

Today, the consensus is that Leibniz and Newton independently invented and described calculus in Europe in the 17th century. Their work was noted to be more than just a "synthesis of previously distinct pieces of mathematical technique, but it was certainly this in part".

It was certainly Isaac Newton who first devised a new infinitesimal calculus and elaborated it into a widely extensible algorithm, whose potentialities he fully understood; of equal certainty, differential and integral calculus, the fount of great developments flowing continuously from 1684 to the present day, was created independently by Gottfried Leibniz.

— Hall 1980: 1

One author has identified the dispute as being about "profoundly different" methods:

Despite ... points of resemblance, the methods [of Newton and Leibniz] are profoundly different, so making the priority row a nonsense.

— Grattan-Guinness 1997: 247

On the other hand, other authors have emphasized the equivalences and mutual translatability of the methods; here Niccolò Guicciardini (2003) appears to confirm L'Hôpital (1696) (already cited):

the Newtonian and Leibnizian schools shared a common mathematical method. They adopted two algorithms, the analytical method of fluxions, and the differential and integral calculus, which were translatable one into the other.

— Guicciardini 2003, on page 250

Scientific priority in the 17th century

In the 17th century, the question of scientific priority was of great importance to scientists; however, during this period, scientific journals had only just begun to appear, and a generally accepted mechanism for establishing priority when publishing discoveries had not yet formed. Among the methods used by scientists were anagrams, sealed envelopes placed in safekeeping, correspondence with other scientists, or private messages. For a French scientist, a letter to Marin Mersenne (the founder of the French Academy of Sciences), or for an English scientist, a letter to Henry Oldenburg (the secretary of the Royal Society of London), essentially carried the status of a published article. The discoverer could "time-stamp" the moment of his discovery and prove that he knew of it at the point the letter was sealed, demonstrating that it had not been copied from anything subsequently published. Nevertheless, if an idea was later published alongside its use in a particularly valuable context, this might take priority over an earlier discoverer's work that had no obvious application. Further, a mathematician's claim could be undermined by counter-claims that he had not truly invented an idea but merely improved on someone else's work—an improvement requiring little skill and based on facts that were already known.

A series of high-profile disputes about scientific priority in the 17th century—an era that the American science historian D. Meli called "the golden age of the mud-slinging priority disputes"—is associated with Leibniz. The first of these occurred at the beginning of 1673 during his first visit to London, when in the presence of the famous mathematician John Pell, he presented his method of approximating series by differences. When Pell remarked that this discovery had already been made by François Regnaud and published in 1670 in Lyon by Gabriel Mouton, Leibniz answered the next day. In a letter to Oldenburg, he wrote that after reviewing Mouton's book, he acknowledged that Pell was correct, but he added that he could provide his draft notes containing nuances not found by Regnaud and Mouton. Thus, the integrity of Leibniz was proven, though this case was recalled later.

During the same visit to London, Leibniz found himself in the opposite position. On 1 February 1673, at a meeting of the Royal Society of London, he demonstrated his mechanical calculator. The Society's curator of experiments, Robert Hooke, carefully examined the device and even removed the back cover. A few days later, in the absence of Leibniz, Hooke criticized the German scientist's machine, claiming he could make a simpler model. Leibniz, who learned about this after returning to Paris, categorically rejected Hooke's claim in a letter to Oldenburg and formulated principles of correct scientific behavior: "We know that respectable and modest people prefer it when they think of something that is consistent with what someone else discovered, to ascribe their own improvements and additions to the discoverer, so as not to arouse suspicions of intellectual dishonesty; the desire for true generosity should pursue them, instead of the lying thirst for dishonest profit." To illustrate proper behavior, Leibniz gave the examples of Nicolas-Claude Fabri de Peiresc and Pierre Gassendi, who performed astronomical observations similar to those made earlier by Galileo Galilei and Johannes Hevelius, respectively. Learning they did not make their discoveries first, the French scientists passed their data on to the original discoverers.

Newton's approach to priority disputes can be illustrated by his discovery of the inverse-square law as applied to the dynamics of bodies moving under the influence of gravity. Based on an analysis of Kepler's laws and his own calculations, Robert Hooke postulated that motion under such conditions should occur along elliptical orbits. Unable to rigorously prove this claim, he reported it to Newton. Without entering into further correspondence with Hooke, Newton solved the problem as well as its inverse, proving that the law of inverse squares follows from the ellipticity of orbits. This discovery was set forth in his famous work Philosophiæ Naturalis Principia Mathematica without mentioning Hooke. At the insistence of astronomer Edmond Halley, to whom the manuscript was handed over for editing and publication, a phrase was included stating that the compliance of Kepler's first law with the law of inverse squares was "independently approved by Wren, Hooke and Halley."

According to a remark by Vladimir Arnold, when choosing between refusing to publish his discoveries and a constant struggle for priority, Newton chose both.

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