Lecture 8. Today we discussed solutions to the wave equation, which arises for A^\mu in the Lorentz gauge with no sources, as well as many other physical contexts. We went through the rationale of separation of variables for such a partial differential equation. We found solutions A(x,y,z,t) = T(t)X(x)Y(y)Z(z), where each function T(t), X(x), etc., solves an ordinary simple harmonic oscillator equation. The arguments of the resulting sinusoidal solutions for X, Y, Z, and T were k_x x, k_y y, k_z z, and c|\vec{k}| t, respectively. We multiplied them to get solutions of the general form A_{\vec{k}} = a_{\vec{k}} exp{i (\omega t - \vec{k}\dot\vec{x}) } + complex conjugate where \vec{k} is any spatial vector, \omega = c|\vec{k}|, and a_\vec{k} is an arbitrary constant coefficient. We discussed why these solutions describe waves: instantaneously, A_{\vec{k}} has a sinusoidal waveform. A point at a particular point on that waveform has phase \phi = \omega t - kx (for \vec{k} taken in the x-direction). Thus the phase stays constant if the point moves forward with velocity \omega/k = c. Thus as we watch time advance the waveform shape moves forward at a velocity c. We then constructed the most general solution to the wave equation. Because the wave equation is linear, the principle of superposition holds --- sums of solutions are solutions. In fact the A_\vec{k} form a complete, orthogonal basis of solutions: any solution of the wave equation can be written as a sum of A_\vec{k}, with particular coefficients a_\vec{k}. A snapshot of that sum at a particular time just gives the Fourier decomposition of the instantaneous field; then the phase (\omega t - \vec{k} \dot \vec{x}) just prescribes how each Fourier component evolves in time, to obey the wave equation. We finally wrote these solutions A_\vec{k} in covariant form. We claimed that, since a particle whose field obeys a wave equation is massless, the particle's energy is just |\vec{p}|c (the rest mass contribution vanishes). Thus we take k^\mu = (|\vec{k}|, \vec{k}) to be the momentum 4-vector of a photon with momentum \vec{k}. We lower this to find the covector k_\mu = = (|\vec{k}|, - \vec{k}). We can then read off how these components appear in the phase of our solutions as A_{\vec{k}} = a_{\vec{k}} exp{i k_\mu x^\mu } + complex conjugate , a manifestly Lorentz covariant form. --- KB