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== 18th-century developments == [[File:Alessandro Volta.jpeg|thumb|upright|[[Alessandro Volta]] (1745–1827)]] During the 18th century, the mechanics founded by Newton was developed by several scientists as more mathematicians learned calculus and elaborated upon its initial formulation. The application of mathematical analysis to problems of motion was known as rational mechanics, or mixed mathematics (and was later termed [[classical mechanics]]). ===Mechanics=== [[File:ETH-BIB-Bernoulli, Daniel (1700-1782)-Portrait-Portr 10971.tif (cropped).jpg|thumb|upright|left|[[Daniel Bernoulli]] (1700–1782)]] In 1714, [[Brook Taylor]] derived the [[fundamental frequency]] of a stretched vibrating string in terms of its tension and mass per unit length by solving a [[differential equation]]. The Swiss mathematician [[Daniel Bernoulli]] (1700–1782) made important mathematical studies of the behavior of gases, anticipating the kinetic theory of gases developed more than a century later, and has been referred to as the first mathematical physicist.<ref>{{Harvtxt|Darrigol|2005}}</ref> In 1733, [[Daniel Bernoulli]] derived the fundamental frequency and [[harmonic]]s of a hanging chain by solving a differential equation. In 1734, Bernoulli solved the differential equation for the vibrations of an elastic bar clamped at one end. Bernoulli's treatment of [[fluid dynamics]] and his examination of [[fluid]] flow was introduced in his 1738 work ''[[Hydrodynamica]]''. Rational mechanics dealt primarily with the development of elaborate mathematical treatments of observed motions, using Newtonian principles as a basis, and emphasized improving the tractability of complex calculations and developing of legitimate means of analytical approximation. A representative contemporary textbook was published by [[Johann Baptiste Horvath]]. By the end of the century analytical treatments were rigorous enough to verify the stability of the Solar System solely on the basis of Newton's laws without reference to divine intervention – even as deterministic treatments of systems as simple as the [[n-body problem|three body problem]] in gravitation remained intractable.<ref>{{Harvtxt|Bos|1980}}</ref> In 1705, [[Edmond Halley]] predicted the periodicity of [[Halley's Comet]], [[William Herschel]] discovered [[Uranus]] in 1781, and [[Henry Cavendish]] measured the [[gravitational constant]] and determined the mass of the Earth in 1798. In 1783, [[John Michell]] suggested that some objects might be so massive that not even light could escape from them. In 1739, [[Leonhard Euler]] solved the ordinary differential equation for a forced harmonic oscillator and noticed the resonance phenomenon. In 1742, [[Colin Maclaurin]] discovered his [[Maclaurin spheroid|uniformly rotating self-gravitating spheroids]]. In 1742, Benjamin Robins published his ''New Principles in Gunnery'', establishing the science of aerodynamics. British work, carried on by mathematicians such as Taylor and Maclaurin, fell behind Continental developments as the century progressed. Meanwhile, work flourished at scientific academies on the Continent, led by such mathematicians as Bernoulli and Euler, as well as [[Joseph-Louis Lagrange]], [[Pierre-Simon Laplace]], and [[Adrien-Marie Legendre]]. In 1743, [[Jean le Rond d'Alembert]] published his ''Traité de dynamique'', in which he introduced the concept of generalized forces for accelerating systems and systems with constraints, and applied the new idea of [[virtual work]] to solve dynamical problem, now known as [[D'Alembert's principle]], as a rival to Newton's second law of motion. In 1747, [[Pierre Louis Maupertuis]] applied minimum principles to mechanics. In 1759, Euler solved the partial differential equation for the vibration of a rectangular drum. In 1764, Euler examined the partial differential equation for the vibration of a circular drum and found one of the Bessel function solutions. In 1776, [[John Smeaton]] published a paper on experiments relating power, [[work (physics)|work]], [[momentum]] and [[kinetic energy]], and supporting the [[conservation of energy]]. In 1788, Lagrange presented his [[Lagrangian mechanics|equations of motion]] in ''[[Mécanique analytique]]'', in which the whole of mechanics was organized around the principle of virtual work. In 1789, [[Antoine Lavoisier]] stated the law of [[conservation of mass]]. The rational mechanics developed in the 18th century received expositions in both Lagrange's ''Mécanique analytique'' and Laplace's ''[[Traité de mécanique céleste]]'' (1799–1825). ===Thermodynamics=== During the 18th century, thermodynamics was developed through the theories of weightless [[imponderable fluid|"imponderable fluids"]], such as heat ("caloric"), [[electricity]], and [[phlogiston theory|phlogiston]] (which was rapidly overthrown as a concept following [[Antoine-Laurent Lavoisier|Lavoisier's]] identification of [[oxygen]] gas late in the century). Assuming that these concepts were real fluids, their flow could be traced through a mechanical apparatus or chemical reactions. This tradition of experimentation led to the development of new kinds of experimental apparatus, such as the [[Leyden Jar]]; and new kinds of measuring instruments, such as the [[calorimeter]], and improved versions of old ones, such as the [[thermometer]]. Experiments also produced new concepts, such as the [[University of Glasgow]] experimenter [[Joseph Black]]'s notion of [[latent heat]] and Philadelphia intellectual [[Benjamin Franklin]]'s characterization of electrical fluid as flowing between places of excess and deficit (a concept later reinterpreted in terms of positive and negative [[electric charge|charges]]). Franklin also showed that lightning is electricity in 1752. The accepted theory of heat in the 18th century viewed it as a kind of fluid, called [[caloric theory|caloric]]; although this theory was later shown to be erroneous, a number of scientists adhering to it nevertheless made important discoveries useful in developing the modern theory, including [[Joseph Black]] (1728–1799) and [[Henry Cavendish]] (1731–1810). Opposed to this caloric theory, which had been developed mainly by the chemists, was the less accepted theory dating from Newton's time that heat is due to the motions of the particles of a substance. This mechanical theory gained support in 1798 from the cannon-boring experiments of Count Rumford ([[Benjamin Thompson]]), who found a direct relationship between heat and mechanical energy. While it was recognized early in the 18th century that finding absolute theories of electrostatic and magnetic force akin to Newton's principles of motion would be an important achievement, none were forthcoming. This impossibility only slowly disappeared as experimental practice became more widespread and more refined in the early years of the 19th century in places such as the newly established [[Royal Institution]] in London. Meanwhile, the analytical methods of rational mechanics began to be applied to experimental phenomena, most influentially with the French mathematician [[Joseph Fourier]]'s analytical treatment of the flow of heat, as published in 1822.<ref>{{Harvtxt|Heilbron|1979}}</ref><ref>{{Harvtxt|Buchwald|1989}}</ref><ref>{{Harvtxt|Golinski|1999}}</ref> [[Joseph Priestley]] proposed an electrical inverse-square law in 1767, and [[Charles-Augustin de Coulomb]] introduced the inverse-square law of [[electrostatics]] in 1798. At the end of the century, the members of the [[French Academy of Sciences]] had attained clear dominance in the field.<ref name="Guicciardini1999" /><ref>{{Harvtxt|Greenberg|1986}}</ref><ref>{{Harvtxt|Guicciardini|1989}}</ref><ref>{{Harvtxt|Garber|1999}}</ref> At the same time, the experimental tradition established by Galileo and his followers persisted. The [[Royal Society]] and the [[French Academy of Sciences]] were major centers for the performance and reporting of experimental work. Experiments in mechanics, optics, [[magnetism]], [[static electricity]], [[history of chemistry|chemistry]], and [[physiology]] were not clearly distinguished from each other during the 18th century, but significant differences in explanatory schemes and, thus, experiment design were emerging. Chemical experimenters, for instance, defied attempts to enforce a scheme of abstract Newtonian forces onto chemical affiliations, and instead focused on the isolation and classification of chemical substances and reactions.<ref>{{Harvtxt|Ben-Chaim|2004}}</ref> {{clear left}}
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