Interference/diffraction

Consider the superposition of two electromagnetic waves.

E1=A1cos(ωtkz+ϕ1)x^E2=A2cos(ωtkz+ϕ2)x^E=E1+E2. \begin{align*} \mathbf E_1 &= A_1 \cos(\omega t - kz + \phi_1) \xhat \\ \mathbf E_2 &= A_2 \cos(\omega t - kz +\phi_2) \xhat \\ \mathbf E &= \mathbf E_1 + \mathbf E_2. \end{align*}

We do not usually measure the electric field of a wave directly, so let’s consider the intensity instead.

I=S=1μ0E×B=nμ0cE2=cnϵ0E2E2 \begin{align*} I = |\mathbf S| = \frac{1}{\mu_0}|\mathbf E \times \mathbf B| = \frac{n}{\mu_0 c} |\mathbf E^2| = cn\epsilon_0 |\mathbf E^2| \propto |\mathbf E^2| \end{align*}

where n=c/vn = c/v is the index of refraction of the material. We calculate IE2I \propto |\mathbf E^2| for our given waves.

E2=E12+E22+2E1E2=A12cos2(ωtkz+ϕ1)+A22cos2(ωt+kz+ϕ2)+2A1A2cos(ωt+kz+ϕ1)cos(ωt+kz+ϕ2). \begin{align*} |\mathbf E^2| &= |\mathbf E_1|^2 + |\mathbf E_2|^2 + 2|\mathbf E_1 \mathbf E_2| \\ &= A_1^2 \cos^2(\omega t - kz + \phi_1) + A_2^2 \cos^2(\omega t + kz + \phi_2)\\ &+ 2A_1A_2 \cos(\omega t + kz + \phi_1) \cos (\omega t + kz + \phi_2). \end{align*}

Taking the time average,

I1T0TE2dt=1μ0(A122+A222+A1A2cos(ϕ1ϕ2)). \begin{align*} \langle I \rangle \propto \frac{1}{T} \int_0^T |\mathbf E^2| \mathrm dt = \frac{1}{\mu_0} \left(\frac{A_1^2}{2} + \frac{A_2^2}{2} + A_1A_2 \cos(\phi_1 - \phi_2) \right). \end{align*}

The plot below shows this time average intensity in terms of the phase difference δ:=ϕ1ϕ2\delta := \phi_1 - \phi_2. We see that when δ\delta is an odd multiple of π\pi the amplitude is at a minimum, and when δ\delta is an even multiple of π\pi, a maximum.

Interference at a material boundary

Consider the boundary between two materials, e.g., the boundary between air and water in a soap bubble. The figure below shows three regions, the air outside the bubble to the left, the water in the middle, and the air inside the bubble to the right. An incident light beam is normal to the boundary, shining from the left. We wish to find the intensity of the reflected light.

A component R1R_1 of the incident light reflects off the outer boundary immediately. Another component R2R_2 is transmitted through the first boundary, then reflected off the second, and finally transmitted again through the first. After a few reflections the intensity of the light decreases significantly, so we will ignore all but R1R_1 and R2R_2.

We use the reflection and transmission coefficients to calculate the amplitude of R1R_1 and R2R_2 relative to the incident beam E0E_0.

R12=n1n2n1+n2T12=2n1n1+n2,R21=n2n1n2+n1,T21=2n2n2+n1R1=R12E0R2=T12R21T21E0. \begin{align*} R_{12} &= \frac{n_1-n_2}{n_1+n_2} \\ T_{12} &= \frac{2n_1}{n_1+n_2}, \quad R_{21} = \frac{n_2-n_1}{n_2+n_1}, \quad T_{21} = \frac{2n_2}{n_2+n_1} \\ R_1 &= R_{12} E_0 \\ R_2 &= T_{12} R_{21} T_{21} E_0. \end{align*}

Since n2>n1n_2>n_1, the reflection off the first boundary R12<0R_{12} < 0, which mean that R1R_1 is negative. This sign flip corresponds to a 180°180\degree phase shift.

R2R_2 has to travel an extra distance 2d2d compared to R1R_1. We have seen that the phase difference due to extra distance traveled is δ=2dk\delta = 2dk. However, it is important to consider that kk depends on the medium.

Let k0k_0 be the wavenumber of the wave in a vacuum. Assuming a non-dispersive wave, ω=vpk\omega = v_p k. The speed of light in material is vn=c/nv_n = c/n, where nn is the index of refraction. Then the wavenumber in material kn=ω/vp,n=ωn/c=nk0k_n = \omega/v_{p,n} = \omega n/c = n k_0.

This means the total phase shift between R1R_1 and R2R_2 is δ=2dkn2π\delta = 2dkn_2 - \pi (or equivalently, +π+\pi, since a phase shift of +π+\pi is exactly the same as a phase shift of π-\pi).

If the incident beam is not normal to the surface, the extra distance traveled will be greater than 2d2d. In the case shown below, the extra distance traveled by R2R_2 is 2d/cosθ2d/\cos\theta'.

Double slit experiment

Consider two small slits a distance dd apart in a thin wall allowing light to shine through onto a wall a distance LL away. We will consider the electric field at a point PP on that wall, an angle θ\theta from the bottom slit.

We assume that LdL \gg d, so E1\mathbf E_1 and E2\mathbf E_2 are roughly parallel (the figure above is greatly exagerated). Then we see that the extra distance the light has to travel from BB to PP is dsinθd\sin\theta (shown in green\color{teal}\text{green}). Assume the electric waves take the form E0cos(krωt)\mathbf E_0 \cos(kr-\omega t), then the phase difference δ=kdsinθ\delta = kd\sin\theta.

As we saw above, we get constructive interference when δ\delta is an even multiple of π\pi, and destructive when it is an odd multiple.

We now extend this experiment to consider the interference from NN slits.

As before, each slit is a distance dd apart, and we consider a point PP far away, such that the line from each slit to PP is roughly parallel, at an angle θ\theta from the horizontal. By the same reasoning as above, the extra distance that light from slit jj must travel relative to slit 11 is jdsinθj d \sin \theta.

We can write the resulting electric field at PP as a superposition of the field from each slit

Etotal=E0[ei(krωt)+ei(krωt+δ)++ei(krωt+(N1)δ)]=E0ei(krωt)j=0N1(eiδ)j=E0ei(krωt)(1eiδN1eiδ)where δ=2πdsinθλ. \begin{align*} E_\text{total} &= E_0 \left[e^{i(\mathbf k \cdot \mathbf r-\omega t)} + e^{i(\mathbf k \cdot \mathbf r - \omega t + \delta)} + \cdots + e^{i(\mathbf k \cdot \mathbf r - \omega t + (N-1)\delta)}\right] \\ &= E_0 e^{i(\mathbf k \cdot \mathbf r - \omega t)} \sum_{j=0}^{N-1} \left(e^{i\delta}\right)^j = E_0 e^{i(\mathbf k \cdot \mathbf r - \omega t)} \left(\frac{1-e^{i\delta N}}{1-e^{i\delta}} \right) \\ \text{where } \delta &= \frac{2\pi d\sin\theta}{\lambda}. \end{align*}

We factor the fraction and simplify to find

1eiδN1eiδ=eiδN/2eiδ/2eiδN/2eiδN/2eiδ/2eiδ/2=eiδ(N1)/2(sin(δN/2)sin(δ/2))Etotal=E0ei(krωt)eiδ(N1)/2(sin(δN/2)sin(δ/2)). \begin{align*} \frac{1-e^{i\delta N}}{1-e^{i\delta}} &= \frac{e^{i\delta N/2}}{e^{i\delta/2}} \cdot \frac{e^{-i\delta N/2} - e^{i\delta N/2}}{e^{-i\delta/2} - e^{i\delta/2}} \\ &= e^{i\delta(N-1)/2} \left(\frac{\sin(\delta N/2)}{\sin(\delta/2)}\right) \\ E_\text{total} &= E_0 e^{i(\mathbf k \cdot \mathbf r - \omega t)} e^{i\delta(N-1)/2} \left(\frac{\sin(\delta N/2)}{\sin(\delta/2)}\right). \end{align*}

The resulting intensity at PP is then

IE2=I0(sin(Nδ/2)sin(δ/2))2. \begin{align*} \langle I\rangle &\propto |E|^2 = I_0 \left(\frac{\sin(N\delta/2)}{\sin(\delta/2)}\right)^2. \end{align*}

The intensity as a function of δ\delta (with N=4N=4) is plotted below.

Note a few things about this plot:

  • We have “principle maxima” at multiples of 2π2\pi, and for N>2N>2 we also have smaller maxima and minima in between.

  • We have N1N-1 minima between adjacent principle maxima.

  • As NN increases, the width of the principle maxima decreases.

  • We can find the width of the principle maxima by finding the first minima.

Infinite slits (diffraction)

We have considered slits of infinitesimal width, which isn’t very physical. We would like to represent slits with some finite width. One way to do this is to consider an infinite set of these infinitesimal slits very close together. This is similar to what we did when moving from discrete coupled oscillators to continuous oscillators.

We start with the same sum as before

Etotal=E0ei(krωt)j=0N1(eiδ)j. E_{\text{total}} = E_0e^{i(\mathbf k \cdot \mathbf r - \omega t)} \sum_{j=0}^{N-1} \left(e^{i\delta} \right)^j.

Instead of a discrete index jj we will use a continuous variable yy to represent the position of each infinitesimal slit.

Etotal=E0ei(krωt)yeiδ(y)where δ(y):=2πysinθλ. \begin{align*} E_\text{total} &= E_0 e^{i(\mathbf k \cdot \mathbf r - \omega t)} \sum_y^\infty e^{i\delta(y)} \\ \text{where } \delta(y) &:= \frac{2\pi y\sin\theta}{\lambda}. \end{align*}

We now define a function S(y)S(y) to describe the shape of our slit. When S(y)=0S(y)=0 none of the incident electric field passes through, and when S(y)=1S(y)=1 all of the field passes through. We use SS to write the electric field as an integral

Etotal=E0ei(krωt)S(y)eiKy ⁣dywhere K=2πsinθλ. \begin{align*} E_\text{total} &= E_0 e^{i(\mathbf k \cdot \mathbf r - \omega t)} \int_{-\infty} ^\infty S(y) e^{-i \mathcal K y} \d y \\ \text{where } \mathcal K &= -\frac{2\pi \sin\theta}{\lambda}. \end{align*}

We see that EtotalE_\text{total} is the Fourier transform of SS.

As usual, we are more interested in intensity than electric field. We can write intensity as

I=I0[S(y)eiKy ⁣dy]2. I = I_0 \left[ \int_{-\infty}^\infty S(y) e^{-i\mathcal Ky} \d y\right]^2.

Let’s evaluate this intensity for a few different slit functions and see what it gives us.

When we have a single wide slit, we get a sinc\mathrm{sinc} pattern.

S(y)={1y<a/20otherwiseI=I0sinc2(aπsinθ/λ). \begin{align*} S(y) &= \begin{cases} 1 & |y| < a/2 \\ 0 & \text{otherwise} \end{cases} \\ I &= I_0 \, \mathrm{sinc}^2 (a\pi\sin\theta/\lambda). \end{align*}

When we have two infinitesimal slits, we get an oscillating intensity. (The plot is not able to show the delta functions well).

S(y)=δ(yd/2)+δ(y+d/2)I=I0cos(πdsinθλ). \begin{align*} S(y) &= \delta(y-d/2) + \delta(y+d/2) \\ I &= I_0 \cos\left(\frac{\pi d \sin\theta}{\lambda}\right). \end{align*}

When we have two thin slits, the result is a product of the previous two results. The width of the slits determines the large-scale pattern, while the distance between them determines the small-scale oscillations.

S(y)={1y±d/2<a/20otherwiseI=I0sinc2(aπsinθλ)cos2(πdsinθλ). \begin{align*} S(y) &= \begin{cases} 1 & |y \pm d/2| < a/2 \\ 0 & \text{otherwise} \end{cases} \\ I &= I_0\, \mathrm{sinc}^2\left(\frac{a\pi\sin\theta}{\lambda}\right)\cos^2\left(\frac{\pi d \sin\theta}{\lambda}\right). \end{align*}

Notice a few things about the solutions:

  • II and SS are Fourier pairs, so yy and K\mathcal K are reciprocal variables. This means that a greater yy corresponds to a smaller K\mathcal K, and vice-versa. For example, a narrower slit will lead to a greater oscillation period in the intensity plot. Two slits closer together will lead to a wider sinc\mathrm{sinc} pattern.

  • Intuitively, if two slits are far apart then it takes only a small change in θ\theta to cause a significant difference in the distance light has to travel from one slit compared to the other. If they are close together, then θ\theta needs to change significantly to cause the same phase difference. This shows why the separation of the slits is inversely related to the period of the intensity oscillations.

Diffraction in two dimensions

A one dimensional slit as we have considered above is still not very physical. Let’s consider how we can extend our calculations to consider a 2D slit function S(x,y)S(x,y).