analysis Fourier analysismathematics

Nowadays, trigonometric series solutions (12) are called Fourier series, after Joseph Fourier, who in 1822 published one of the great mathematical classics, The Analytical Theory of Heat. Fourier began with a problem closely analogous to the vibrating violin string: the conduction of heat in a rigid rod of length l. If T(x, t) denotes the temperature at position x and time t, then it satisfies a partial differential equationT_t = a²T_xx (15)that differs from the wave equation only in having the first time derivative T_t instead of the second, T_tt. This apparently minor change has huge consequences, both mathematical and physical. Again there are boundary conditions, expressing the fact that the temperatures at the ends of the rod are held fixed—for example,T(0, t) = 0 and T(l, t) = 0, (16)if the ends are held at zero temperature. The physical effect of the first time derivative is profound: instead of getting persistent vibrational waves, the heat spreads out more and more smoothly—it diffuses.

Fourier showed that his heat equation can be solved using trigonometric series. He invented a method (now called Fourier analysis) of finding appropriate coefficients a₁, a₂, a₃, … in equation (12) for any given initial temperature distribution. He did not solve the problem of providing rigorous logical foundations for such series—indeed, along with most of his contemporaries, he failed to appreciate the need for such foundations—but he provided major motivation for those who eventually did establish foundations.

These developments were not just of theoretical interest. The wave equation, in particular, is exceedingly important. Waves arise not only in musical instruments but in all sources of sound and in light. Euler found a three-dimensional version of the wave equation, which he applied to sound waves; it takes the formw_tt = c²(w_xx + w_yy + w_zz) (17)where now w(x, y, z, t) is the pressure of the sound wave at point (x, y, z) at time t. The expression w_xx + w_yy + w_zz is called the Laplacian, after the French mathematician Pierre-Simon de Laplace, and is central to classical mathematical physics. Roughly a century after Euler, the Scottish physicist James Clerk Maxwell extracted the three-dimensional wave equation from his equations for electromagnetism, and in consequence he was able to predict the existence of radio waves. It is probably fair to suggest that radio, television, and radar would not exist today without the early mathematicians’ work on the analytic aspects of musical instruments.