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In my studies of geometrical optics, I have encountered variations of the claim that, from what I recall, when the amplitude of the wave is changing slowly, the ray equation is a valid solution to Maxwell's equations, and can therefore be used to evaluate optical systems, or something of the sort. However, this is never elaborated upon, and I'm unsatisfied with my understanding (or lack thereof) of what this really means.

For instance, often accompanying the aforementioned claim is a diagram such as the following:

enter image description here

If my understanding is correct, the ray equation is not valid along the boundaries of the wavefronts in the above diagram, since that's where refraction occurs. But I don't actually understand why this is the case, or, put another way, I don't really appreciate what this means.

Furthermore, I'm not completely sure what qualifies as a boundary of a wavefront in the above diagram. This is made more confusing by the fact that the author of the diagram has drawn lines depicting rays along (what I'm presuming are) the boundaries of the wavefronts, despite the fact that, as I just said, the ray equation is invalid along the boundaries of the wavefronts.

And lastly, what is happening at the focus in such a diagram? Are foci actually boundaries, and, therefore, the ray equation is invalid at foci? And, tying this back into the aforementioned claim, what happens to the amplitude of the wave at such a point?

I would greatly appreciate it if people could please take the time to explain all of this.


EDIT:

I just found the following on page 388 of Electromagnetic Fields, by Jean G. Van Bladel:

An important example of failure occurs when the rays converge to a focus, where the theory predicts an infinite value for the power density of $I$ in (8.101).

This still isn't an explanation, but at least it confirms what I suspected: The ray equation is invalid at foci.

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Consider a packet composed of a roughly uniform train of waves spread out over a region that is substantially longer and wider than their mean wavelength. Any particular point of space and time, ${\bf x}$ and $t$, it has a definite phase $\Theta({\bf x},t)$. Once we know this phase, we can define the local frequency $\omega$ and wave-vector ${\bf k}$ by $$ \omega= -\left(\frac{\partial\Theta}{\partial t}\right)_x,\qquad k_i = \left(\frac{\partial\Theta}{\partial x_i }\right)_t. $$ These definitions are motivated by the idea that $$ \Theta({\bf x},t)\sim {\bf k}\cdot {\bf x} -\omega t, $$ at least locally.

We wish to understand how ${\bf k}$ changes as the wave propagates through a slowly varying medium. Assume that the dispersion equation $\omega=\omega ({\bf k})$, which is initially derived for a uniform medium, can be extended to $\omega =\omega({\bf k}, {\bf x})$, where the $\bf x$ dependence arises, for example, as a result of a position-dependent refractive index. This assumption is only an approximation, but it is a good approximation when the distance over which the medium changes is much larger than the distance between wavecrests.

Applying the equality of mixed partials to the definitions of ${\bf k}$ and $\omega$ gives us $$ \left(\frac{\partial \omega}{\partial x_i }\right)_t= -\left(\frac{\partial k_i}{\partial t }\right)_{\bf x},\quad \left(\frac{\partial k_i}{\partial x_j }\right)_{x_i}= \left(\frac{\partial k_j}{\partial x_i }\right)_{x_j}. \quad (\star) $$ The subscripts indicate what is being left fixed when we differentiate. We must be careful about this, because we want to use the dispersion equation to express $\omega$ as a function of ${\bf k}$ and ${\bf x}$, and the wave-vector ${\bf k}$ will itself be a function of ${\bf x}$ and $t$.

Taking this dependence into account, we write $$ \left(\frac{\partial \omega}{\partial x_i }\right)_t= \left(\frac{\partial \omega}{\partial x_i }\right)_{\bf k} + \left(\frac{\partial \omega}{\partial k_j }\right)_{\bf x}\left(\frac{\partial k_j}{\partial x_i }\right)_t. $$ We now use ($\star$) to rewrite this as $$ \left(\frac{\partial k_i}{\partial t }\right)_{\bf x}+ \left(\frac{\partial \omega}{\partial k_j }\right)_{\bf x}\left(\frac{\partial k_i}{\partial x_j }\right)_t = -\left(\frac{\partial \omega}{\partial x_i }\right)_{\bf k}. $$ Interpreting the left hand side as a convective derivative $$ \frac{dk_i}{dt}=\left(\frac{\partial k_i}{\partial t }\right)_{\bf x}+({\bf V}_g\cdot\nabla) k_i, $$ we read off that
$$ \frac {dk_i}{dt}= -\left(\frac{\partial \omega}{\partial x_i }\right)_{\bf k} $$ provided we are moving at velocity $$ \frac {dx_i}{dt}=({\bf V}_g)_i= \left(\frac{\partial \omega}{\partial k_i }\right)_{\bf x}. $$ Since this is the group velocity, the packet of waves is actually travelling at this speed. The last two equations therefore tell us how the orientation and wavelength of the wave train evolve if we ride along with the packet as it is refracted by the inhomogeneity.

The formulae $$ \dot {\bf k} = -\frac{\partial \omega}{\partial {\bf x} },\\ \dot {\bf x}= \phantom -\frac{\partial \omega}{\partial {\bf k} }, $$ are Hamilton's ray equations and are the basis for geometric optics. These Hamilton equations are identical in form to Hamilton's equations for classical mechanics except that ${\bf k}$ is playing the role of the canonical momentum, ${\bf p}$, and $\omega({\bf k}, {\bf x})$ replaces the Hamiltonian, $H({\bf p}, {\bf x})$.

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  • $\begingroup$ Thanks for the answer. Can you please clarify how you used $\star$ to get $$\left(\frac{\partial k_i}{\partial t }\right)_{\bf x}+ \left(\frac{\partial \omega}{\partial k_j }\right)_{\bf x}\left(\frac{\partial k_i}{\partial x_j }\right)_t = -\left(\frac{\partial \omega}{\partial x_i }\right)_{\bf k}?$$ Also, It's not clear to me that your answer addresses my questions? $\endgroup$ Nov 18, 2019 at 20:32

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