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Fourier Optics

10.1 Fraunhofer Diffraction as a Fourier Transform

The Fraunhofer diffraction pattern of an aperture with transmittance function t(x,y)t(x, y) illuminated by a plane wave is proportional to the 2D Fourier transform of the aperture function:

E(u,v)t(x,y)e2πi(ux+vy)dxdy=F{t(x,y)}(u,v)E(u, v) \propto \iint t(x,y)\, e^{-2\pi i(ux + vy)}\, dx\, dy = \mathcal{F}\{t(x,y)\}(u, v)

Where u=sinθx/λu = \sin\theta_x/\lambda and v=sinθy/λv = \sin\theta_y/\lambda are the spatial frequencies.

Theorem 10.1. The intensity in the Fraunhofer diffraction pattern is

I(u,v)=I0t~(u,v)2I(u,v) = I_0\,|\tilde{t}(u,v)|^2

Where t~(u,v)=F{t(x,y)}(u,v)\tilde{t}(u,v) = \mathcal{F}\{t(x,y)\}(u,v) is the Fourier transform of the aperture function.

Proof. The Huygens-Fresnel principle in the far field gives:

E(x",y)=eikriλrt(x,y)eik(xx+yy)/rdxdyE(x",y') = \frac{e^{ikr}}{i\lambda r}\iint t(x,y)\, e^{-ik(xx' + yy')/r}\, dx\, dy

In the far field, rDr \approx D and the phase factor eik(xx+yy)/re^{-ik(xx' + yy')/r} is exactly the kernel of the Fourier transform. \blacksquare

10.2 Convolution Theorem for Diffraction

Theorem 10.2 (Convolution theorem). If an aperture function is the convolution t=t1t2t = t_1 * t_2The diffraction pattern is the product of the individual diffraction patterns:

F{t1t2}=F{t1}F{t2}\mathcal{F}\{t_1 * t_2\} = \mathcal{F}\{t_1\} \cdot \mathcal{F}\{t_2\}

Corollary. If an aperture is the product t=t1t2t = t_1 \cdot t_2The diffraction pattern is the convolution of the individual patterns:

F{t1t2}=F{t1}F{t2}\mathcal{F}\{t_1 \cdot t_2\} = \mathcal{F}\{t_1\} * \mathcal{F}\{t_2\}

10.3 Worked Example: Diffraction Grating via Fourier Transform

Problem. Use the Fourier transform to derive the intensity pattern of a grating with NN slits of width aa and spacing dd.

Solution

The transmittance of a single slit centred at x=0x = 0 is tslit(x)=rect(x/a)t_{\mathrm{slit}(x) = \mathrm{rect}(x/a)}. The full grating is NN slits:

t(x)=n=0N1tslit(xnd)=tslit(x)n=0N1δ(xnd)t(x) = \sum_{n=0}^{N-1} t_{\mathrm{slit}(x - nd) = t_{\mathrm{slit}(x) * \sum_{n=0}^{N-1} \delta(x - nd)}}

The Fourier transform is:

t~(u)=F{tslit}F{n=0N1δ(xnd)}\tilde{t}(u) = \mathcal{F}\{t_{\mathrm{slit}\} \cdot \mathcal{F}\left\{\sum_{n=0}^{N-1}\delta(x - nd)\right\}}

=asinc(πau)n=0N1e2πindu=asinc(πau)sin(Nπdu)sin(πdu)= a\,\mathrm{sinc}(\pi a u) \cdot \sum_{n=0}^{N-1} e^{-2\pi i n d u} = a\,\mathrm{sinc}(\pi a u) \cdot \frac{\sin(N\pi d u)}{\sin(\pi d u)}

The intensity is:

I(u)=I0a2sinc2(πau)sin2(Nπdu)sin2(πdu)I(u) = I_0\,a^2\,\mathrm{sinc}^2(\pi a u)\,\frac{\sin^2(N\pi d u)}{\sin^2(\pi d u)}

The first factor is the single-slit envelope; the second is the NN-slit interference pattern. Principal maxima occur at du=mdu = m (integer mm), giving the grating equation dsinθ=mλd\sin\theta = m\lambda.

\blacksquare

10.4 Worked Example: Circular Aperture and the Airy Pattern

Problem. Compute the Fraunhofer diffraction pattern of a circular aperture of radius aa.

Solution

The aperture function is t(r)=1t(r) = 1 for rar \leq a and t(r)=0t(r) = 0 for r>ar > a. By circular symmetry, the Fourier transform in polar coordinates is:

t~(q)=2π0aJ0(2πqr)rdr\tilde{t}(q) = 2\pi\int_0^a J_0(2\pi q r)\, r\, dr

Where J0J_0 is the Bessel function of the first kind and q=sinθ/λq = \sin\theta/\lambda is the radial spatial frequency. Using the identity:

0aJ0(2πqr)rdr=a2πqJ1(2πqa)\int_0^a J_0(2\pi q r)\, r\, dr = \frac{a}{2\pi q}J_1(2\pi q a)

t~(q)=πa22J1(α)α\tilde{t}(q) = \pi a^2 \cdot \frac{2J_1(\alpha)}{\alpha}

Where α=2πaq=2πasinθ/λ\alpha = 2\pi a q = 2\pi a\sin\theta/\lambda. The intensity is:

I(θ)=I0(2J1(α)α)2I(\theta) = I_0\left(\frac{2J_1(\alpha)}{\alpha}\right)^2

This is the Airy pattern. The first zero occurs at α=3.832\alpha = 3.832Giving the angular radius of the first dark ring:

sinθ1=1.22λd\sin\theta_1 = 1.22\,\frac{\lambda}{d}

Where d=2ad = 2a is the diameter.

\blacksquare