5.6   Making the Train, Making a Packet


As we noticed earlier, the problem with the sinusoidal waveforms we’ve considered so far, is that they go on for ever. According to our probabilistic model, this effectively would mean that there was an equal chance of a particle being detected anywhere in the universe. Cormorant is quick to point out that this seems like an unpromising starting point for modelling something on the scale of an atom. But Joseph Fourier pipes up from the corner: “Bon courage, petit oiseau! Have you so soon forgotten what I taught you? You can synthesise any waveform you wish if you superpose, superpose and superpose encore.” Joseph announced this incredibly important discovery to the world at the beginning of the 19th century, to a deafening chorus of indifference. Jospeh ranks high in the tragic league table of scientists who went underappreciated in their lifetimes (“Tell me about it” moans Sir Isaac; much coughing and spluttering ensues).   

Joseph showed that almost any smooth, periodic function can be constructed as a sum of series of sine and cosine functions. We’ll take a simplified, special case of a Fourier series to explore what this might mean for us.  Figure V-iii shows, for example, what can happen if we superpose a series of cosine curves (which are just sine curves but shifted by π/2 radians, so that they have a peak centred on zero), with different wavelengths. The equation of each of the individual curves is  y  =  cos(2πx/λ), which we can write more concisely as y = cos(kx), where k is 2π/λ, which is officially called the angular wavenumber.