A time-harmonic wave has sinusoidal dependence on time at a single real angular frequency. With the conventionthe spatial complex amplitude contains both local amplitude and wave phase. Differentiation with respect to time becomes multiplication by . Substitution into the uniform wave equation gives the Helmholtz equation , with .
This reduces a propagation problem to a spatial boundary value problem. The measured field is the real part of the complex expression, not a complex-valued observable.[ref]
The Feynman Lectures on Physics, Volume I by Richard Feynman and others. Chapter 23, §23–1: real sinusoidal forces represented by complex exponentials
A radiating solution still needs an outgoing condition; its spatial factors and signs must agree with the selected time convention. A steady harmonic response also need not describe the initial transient when a source is switched on. Articles by others on the same topic
There are currently no matching articles.