Let’s consider what happens when a wave crosses a boundary between materials. We considered this in 1D, and we will now consider it in 2D or 3D.
Assume we have a boundary between two materials at x=0, and an incident wave with wave vector k in the x,y plane coming from the left. Just like in the 1D case, when the wave reaches the boundary we will have a reflected and a transmitted wave.
Let’s consider the boundary conditions. Just as in the 1D case, the waves on either side of the boundary must have the same frequency ω, otherwise there would be discontinuities at the boundary. If the boundary were a membrane, for instance, a discontinuity might correspond to the membrane breaking. Whatever the medium and wave though, the waves on either side need to be continuous.
Consider the following figure showing the wavefronts of an incident and transmitted waves. Because the wavelengths are different on either side of the boundary, the angle of the incident and transmitted wave must be different so that the boundary is continuous
At x=0, ψL=ψR, since the boundary doesn’t break, so
Aei(kyy−ωt)+ARei(kryy−ωt)=ATei(ktyy−ωt).
The only way this can be true for all y is if ky=kry=kty. We can now relate the angular frequency to the wave vectors. Let’s assume both materials are not dispersive, then the dispersion relation is ω=vp∣k∣.
Since ky=kry, we know kx2=krx2. In this case since the boundary is along the y axis, the reflection is flipped in x, so krx=−kx.
Looking at the transmitted wave, we know that the y component kty=ky is the same as the incident wave. We can use this to relate the incident angle θ to the transmitted angle θ′.
In the case of light, we define an index of refraction n:=c/v≈ϵ/ϵ0, (since μ≈μ0 for transparent materials) giving us the relation known as Snell’s law
n1sinθ1=n2sinθ2.
This allows us to relate the transmitted angle to the incident angle. We will now consider how to relate the amplitudes of the incident, reflected, and transmitted waves. The exact behavior at the boundary will depend on the polarization of the incident wave. We can consider the incident light as a superposition of two polarization states; we will consider each separately.
P-polarization
The P-polarized component of the incident wave is at some angle from the boundary, its electric field shown in the figure.
We further break down this electric field into the components perpendicular and parallel to the boundary. First consider the perpendicular component (here the boundary is the plane in/out of the page).
We apply Gauss’s law at the boundary over the volume shown with cross sectional area A and depth d. In the limit as d→0 the enclosed charge ρ goes to zero,
∬ϵE⋅dA=ϵ1AEP⊥1−ϵ2AEP⊥2=0.
Which gives us ϵ1EP⊥1=ϵ2EP⊥2.
Now consider the parallel component.
We apply Faraday’s law along the contour highlighted above. In the limit as d→0, the magnetic flux ΦB goes to zero,
∮E⋅ds=lEP∥1−lEP∥2=−dtd0=0.
Which gives us EP∥1=EP∥2.
We now use these conditions in combination with Snell’s law to relate theincident EP,i, reflected EP,r and transmitted EP,t amplitudes of the (P-polarized) waves.
When θ=90° (parallel to the boundary), α→∞, R→1, T→0, so there is no transmission.
S-polarization
The S-polarized component of the incident wave is in the plane of the boundary, its electric field shown pointing in and out of the page in the figure.
Considering the magnetic fields we can do a similar derivation to what we did above.