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411. Integral of equation (e) of vibrating elastic surfaces

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413. Use of the same theorem to obtain the integrals, by summing the
series which represent them. Application to the equation

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Integral under finite form containing two arbitrary functions of t.
414. The expressions change form when we use other limits of the definite

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integrals
415, 416. Construction which serves to prove the general equation

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the second member of which represents a periodic function

419. The chief character of the theorem expressed by equation (B) consists
in this, that the sign ƒ of the function is transferred to another unknown
a, and that the chief variable x is only under the symbol cosine

420. Use of these theorems in the analysis of imaginary quantities

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423. Construction which serves to prove the general equation. Consequences
relative to the extent of equations of this kind, to the values of ƒ (x)
which correspond to the limits of x, to the infinite values of ƒ (x)

424-427. The method which consists in determining by definite integrals

the unknown coefficients of the development of a function of x under

the form

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PRELIMINARY DISCOURSE.

PRIMARY causes are unknown to us; but are subject to simple and constant laws, which may be discovered by observation, the study of them being the object of natural philosophy.

Heat, like gravity, penetrates every substance of the universe, its rays occupy all parts of space. The object of our work is to set forth the mathematical laws which this element obeys. The theory of heat will hereafter form one of the most important branches of general physics.

The knowledge of rational mechanics, which the most ancient nations had been able to acquire, has not come down to us, and the history of this science, if we except the first theorems in harmony, is not traced up beyond the discoveries of Archimedes. This great geometer explained the mathematical principles of the equilibrium of solids and fluids. About eighteen centuries elapsed before Galileo, the originator of dynamical theories, discovered the laws of motion of heavy bodies. Within this new science Newton comprised the whole system of the universe. The successors of these philosophers have extended these theories, and given them an admirable perfection: they have taught us that the most diverse phenomena are subject to a small number of fundamental laws which are reproduced in all the acts of nature. It is recognised that the same principles regulate all the movements of the stars, their form, the inequalities of their courses, the equilibrium and the oscillations of the seas, the harmonic vibrations of air and sonorous bodies, the transmission of light, capillary actions, the undulations of fluids, in fine the most complex effects of all the natural forces, and thus has the thought

F. H.

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