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The Timpson Lyceum · University Physics II (2026) – Electricity & Magnetism

Chapter 36 — Diffraction

Problems with worked solutions · 14 points · 3 extra credit

Chapter 36 — Diffraction

Core: 14 points · Extra credit: 3 points. Show your reasoning; partial credit is given.

  1. 1. (2 pts ••) Monochromatic light of wavelength λ=633 nm\lambda=633\,\text{nm} from a helium–neon laser passes through a single slit of width a=0.12 mma=0.12\,\text{mm} and forms a diffraction pattern on a screen L=2.5 mL=2.5\,\text{m} away. The angles are small enough that sin⁡θ≈tan⁡θ\sin\theta\approx\tan\theta.

    (a) Find the angle to the first dark fringe (m=1m=1).

    (b) Find the distance on the screen from the center of the pattern to the first dark fringe.

    (c) Find the full width of the central bright band (the distance between the first dark fringes on either side).

    Solution

    1.

    (a) First dark fringe: asin⁡θ=λa\sin\theta=\lambda, so sin⁡θ=λa=633×10−90.12×10−3=5.28×10−3\sin\theta=\dfrac{\lambda}{a}=\dfrac{633\times10^{-9}}{0.12\times10^{-3}}=5.28\times10^{-3}, giving θ≈0.30∘\theta\approx0.30^\circ (5.3×10−3 rad5.3\times10^{-3}\,\text{rad}).

    (b) With small angles, y1=Ltan⁡θ≈Lsin⁡θ=(2.5)(5.28×10−3)≈1.3×10−2 m=13 mmy_1=L\tan\theta\approx L\sin\theta=(2.5)(5.28\times10^{-3})\approx1.3\times10^{-2}\,\text{m}=13\,\text{mm}.

    (c) The central band runs from the m=−1m=-1 to the m=+1m=+1 dark fringe, so its full width is 2y1≈2(13 mm)≈26 mm2y_1\approx2(13\,\text{mm})\approx26\,\text{mm}.

  2. 2. (2 pts ••) A single slit of width a=0.15 mma=0.15\,\text{mm} is illuminated by light of wavelength λ=600 nm\lambda=600\,\text{nm}. The intensity as a function of the diffraction angle is

    I=I0[sin⁡(β/2)β/2]2,β=2πaλsin⁡θ.I=I_0\left[\frac{\sin(\beta/2)}{\beta/2}\right]^2,\qquad \beta=\frac{2\pi a}{\lambda}\sin\theta .

    (a) Find the angle at which β/2=π/2\beta/2=\pi/2 (i.e. halfway, in the phase variable, to the first minimum).

    (b) Find the intensity at that angle as a fraction of the central intensity I0I_0.

    (c) The first secondary maximum occurs near β/2=1.43π\beta/2=1.43\pi. Find its intensity as a fraction of I0I_0, and comment on how much dimmer it is than the central peak.

    Solution

    2.

    (a) β/2=πaλsin⁡θ=π2\beta/2=\dfrac{\pi a}{\lambda}\sin\theta=\dfrac{\pi}{2} requires sin⁡θ=λ2a=600×10−92(0.15×10−3)=2.0×10−3\sin\theta=\dfrac{\lambda}{2a}=\dfrac{600\times10^{-9}}{2(0.15\times10^{-3})}=2.0\times10^{-3}, so θ≈0.11∘\theta\approx0.11^\circ.

    (b) II0=[sin⁡(π/2)π/2]2=(1π/2)2=(2π)2≈0.41\dfrac{I}{I_0}=\left[\dfrac{\sin(\pi/2)}{\pi/2}\right]^2=\left(\dfrac{1}{\pi/2}\right)^2=\left(\dfrac{2}{\pi}\right)^2\approx0.41. The intensity has already dropped to about 41%41\% of the peak here.

    (c) At β/2=1.43π\beta/2=1.43\pi: II0=[sin⁡(1.43π)1.43π]2≈(−0.9684.49)2≈0.047\dfrac{I}{I_0}=\left[\dfrac{\sin(1.43\pi)}{1.43\pi}\right]^2\approx\left(\dfrac{-0.968}{4.49}\right)^2\approx0.047. The first side lobe carries only about 4.7%4.7\% of the central intensity — the central peak dominates by more than a factor of 2020.

  3. 3. (2 pts ••) A diffraction grating has 600600 lines per millimetre and is illuminated at normal incidence by sodium light, λ=589 nm\lambda=589\,\text{nm}.

    (a) Find the slit spacing dd.

    (b) Find the diffraction angles of the first- and second-order bright fringes.

    (c) What is the highest order that can be observed with this grating and wavelength? Explain.

    Solution

    3.

    (a) d=1 mm600=1.667×10−3 mm=1.67×10−6 md=\dfrac{1\,\text{mm}}{600}=1.667\times10^{-3}\,\text{mm}=1.67\times10^{-6}\,\text{m} (1667 nm1667\,\text{nm}).

    (b) sin⁡θm=mλd\sin\theta_m=\dfrac{m\lambda}{d}.

    m=1m=1: sin⁡θ1=589×10−91.667×10−6=0.3534\sin\theta_1=\dfrac{589\times10^{-9}}{1.667\times10^{-6}}=0.3534, so θ1≈20.7∘\theta_1\approx20.7^\circ.

    m=2m=2: sin⁡θ2=0.7068\sin\theta_2=0.7068, so θ2≈45.0∘\theta_2\approx45.0^\circ.

    (c) The largest possible order has sin⁡θ≤1\sin\theta\le1: mmax⁡=dλ=1.667×10−6589×10−9=2.83m_{\max}=\dfrac{d}{\lambda}=\dfrac{1.667\times10^{-6}}{589\times10^{-9}}=2.83. Since mm must be an integer, the highest observable order is m=2m=2. (Order 33 would need sin⁡θ=1.06>1\sin\theta=1.06>1, which is impossible.)

  4. 4. (2 pts ••) The sodium doublet consists of two closely spaced lines at λ1=589.00 nm\lambda_1=589.00\,\text{nm} and λ2=589.59 nm\lambda_2=589.59\,\text{nm}. The resolving power of a grating is R=NmR=Nm, where NN is the number of illuminated slits and mm is the order.

    (a) What resolving power is needed to just separate the two lines?

    (b) Working in second order (m=2m=2), how many slits must be illuminated?

    (c) If the grating has 600600 lines per millimetre, what width of the grating must the beam cover to achieve this?

    Solution

    4.

    (a) R=λΔλ=589.000.59≈1.0×103R=\dfrac{\lambda}{\Delta\lambda}=\dfrac{589.00}{0.59}\approx1.0\times10^{3} (about 998998).

    (b) N=Rm=9982≈5.0×102N=\dfrac{R}{m}=\dfrac{998}{2}\approx5.0\times10^{2} slits (about 499499).

    (c) At 600600 lines per mm, NN slits span N600 mm=499600≈0.83 mm\dfrac{N}{600}\,\text{mm}=\dfrac{499}{600}\approx0.83\,\text{mm}. A beam covering roughly 0.83 mm0.83\,\text{mm} of the grating suffices.

  5. 5. (2 pts ••) A camera lens and a telescope are limited by the diffraction of a circular aperture; the Rayleigh criterion gives the smallest resolvable angular separation as θ=1.22 λ/D\theta=1.22\,\lambda/D. Take λ=550 nm\lambda=550\,\text{nm} throughout.

    (a) A space telescope has a primary mirror of diameter D=2.4 mD=2.4\,\text{m}. Find its diffraction-limited angular resolution, in radians and in arcseconds.

    (b) Aimed at the Moon (3.84×108 m3.84\times10^{8}\,\text{m} away), what is the smallest surface separation it could resolve?

    (c) The dark-adapted human eye has a pupil of diameter D=3.0 mmD=3.0\,\text{mm}. How far away can two headlights separated by 1.5 m1.5\,\text{m} be and still be resolved as two sources?

    Solution

    5.

    (a) θ=1.22λD=1.22(550×10−9)2.4=2.80×10−7 rad\theta=\dfrac{1.22\lambda}{D}=\dfrac{1.22(550\times10^{-9})}{2.4}=2.80\times10^{-7}\,\text{rad}. In arcseconds: (2.80×10−7)(180π)(3600)≈0.058′′(2.80\times10^{-7})\left(\dfrac{180}{\pi}\right)(3600)\approx0.058''.

    (b) s=θ L=(2.80×10−7)(3.84×108)≈1.1×102 ms=\theta\,L=(2.80\times10^{-7})(3.84\times10^{8})\approx1.1\times10^{2}\,\text{m} (about 107 m107\,\text{m}).

    (c) θ=1.22(550×10−9)3.0×10−3=2.24×10−4 rad\theta=\dfrac{1.22(550\times10^{-9})}{3.0\times10^{-3}}=2.24\times10^{-4}\,\text{rad}. The headlights subtend this angle at distance L=sθ=1.52.24×10−4≈6.7×103 m≈6.7 kmL=\dfrac{s}{\theta}=\dfrac{1.5}{2.24\times10^{-4}}\approx6.7\times10^{3}\,\text{m}\approx6.7\,\text{km}. (Real eyes do far worse; diffraction is only the theoretical limit.)

  6. 6. (2 pts ••) X-rays are directed at a crystal of table salt (NaCl), whose atomic planes are separated by d=0.282 nmd=0.282\,\text{nm}. A strong first-order reflection (m=1m=1) is observed when the beam makes a grazing angle of θ=15.9∘\theta=15.9^\circ with the planes. Bragg's law is 2dsin⁡θ=mλ2d\sin\theta=m\lambda.

    (a) Find the wavelength of the X-rays.

    (b) Find the grazing angle at which the second-order reflection (m=2m=2) appears.

    (c) What is the highest order that can be observed with these X-rays and this spacing?

    Solution

    6.

    (a) 2dsin⁡θ=mλ2d\sin\theta=m\lambda with m=1m=1: λ=2dsin⁡θ=2(0.282×10−9)sin⁡15.9∘=2(0.282×10−9)(0.2740)≈1.55×10−10 m=0.154 nm\lambda=2d\sin\theta=2(0.282\times10^{-9})\sin15.9^\circ=2(0.282\times10^{-9})(0.2740)\approx1.55\times10^{-10}\,\text{m}=0.154\,\text{nm}. (This is essentially the copper KαK_\alpha line.)

    (b) m=2m=2: sin⁡θ=2λ2d=2(0.1545×10−9)2(0.282×10−9)=0.15450.282=0.5480\sin\theta=\dfrac{2\lambda}{2d}=\dfrac{2(0.1545\times10^{-9})}{2(0.282\times10^{-9})}=\dfrac{0.1545}{0.282}=0.5480, so θ≈33.2∘\theta\approx33.2^\circ.

    (c) mmax⁡=2dλ=2(0.282×10−9)0.1545×10−9=3.65m_{\max}=\dfrac{2d}{\lambda}=\dfrac{2(0.282\times10^{-9})}{0.1545\times10^{-9}}=3.65, so the highest observable order is m=3m=3 (at sin⁡θ=0.822\sin\theta=0.822, θ≈55.3∘\theta\approx55.3^\circ).

  7. 7. (2 pts ••) A double-slit apparatus has slits of width a=0.050 mma=0.050\,\text{mm} with their centers separated by d=0.25 mmd=0.25\,\text{mm}, illuminated by light of wavelength λ=550 nm\lambda=550\,\text{nm}. The observed pattern is the two-slit interference fringes modulated by the single-slit diffraction envelope.

    (a) At what interference orders mm are bright fringes missing because they fall on a zero of the single-slit envelope? Identify the lowest such order.

    (b) How many bright interference fringes appear within the central diffraction maximum (counting the central fringe and those on both sides, but excluding any that land exactly on the first diffraction minimum)?

    Solution

    7.

    (a) An interference maximum at dsin⁡θ=mλd\sin\theta=m\lambda is missing when it coincides with a diffraction minimum asin⁡θ=pλa\sin\theta=p\lambda. Dividing, the missing orders satisfy mp=da=0.250.050=5\dfrac{m}{p}=\dfrac{d}{a}=\dfrac{0.25}{0.050}=5. So m=5pm=5p: orders m=±5,±10,…m=\pm5,\pm10,\dots are missing. The lowest is m=5m=5.

    (b) The central diffraction maximum extends out to the first diffraction minimum at sin⁡θ=λ/a\sin\theta=\lambda/a. Interference maxima lie at sin⁡θ=mλ/d\sin\theta=m\lambda/d, so they fall inside the central envelope when mλd<λa\dfrac{m\lambda}{d}<\dfrac{\lambda}{a}, i.e. ∣m∣<da=5|m|<\dfrac{d}{a}=5. Thus m=−4,−3,…,3,4m=-4,-3,\dots,3,4: that is 99 bright fringes. (The m=±5m=\pm5 fringes land exactly on the diffraction minimum and are suppressed.)

  8. Extra Credit (3 pts •••)

    Derive the single-slit intensity pattern from scratch using phasor (amplitude) integration.

    Consider a slit of width aa illuminated by a plane wave. Divide the slit into infinitesimal strips of width dydy at position yy (with −a/2≤y≤a/2-a/2\le y\le a/2). Each strip radiates a wavelet toward a distant screen at angle θ\theta; relative to the strip at y=0y=0, the wavelet from the strip at yy has an extra path length ysin⁡θy\sin\theta, hence a phase ϕ(y)=kysin⁡θ\phi(y)=ky\sin\theta with k=2π/λk=2\pi/\lambda. Each strip contributes an amplitude dE0=(E0/a) dydE_0=(E_0/a)\,dy, where E0E_0 is the total amplitude that would arrive with all strips in phase.

    (a) Write the total (complex) field at the screen as the integral E=∫−a/2a/2E0a ei kysin⁡θ dyE=\displaystyle\int_{-a/2}^{a/2}\frac{E_0}{a}\,e^{i\,ky\sin\theta}\,dy, and carry out the integration.

    (b) Show that the magnitude reduces to

    ∣E∣=E0 sin⁡(β/2)β/2,β=2πaλsin⁡θ,|E|=E_0\,\frac{\sin(\beta/2)}{\beta/2},\qquad \beta=\frac{2\pi a}{\lambda}\sin\theta ,

    and hence that the intensity (proportional to ∣E∣2|E|^2) is I=I0[sin⁡(β/2)β/2]2I=I_0\left[\dfrac{\sin(\beta/2)}{\beta/2}\right]^2.

    (c) From this result, show that the minima occur at asin⁡θ=mλa\sin\theta=m\lambda for nonzero integers mm, and use a limit to verify that I→I0I\to I_0 as θ→0\theta\to0.

    Solution

    Extra Credit

    (a) The total field is the sum (integral) of the strip contributions:

    E=∫−a/2a/2E0a ei kysin⁡θ dy.E=\int_{-a/2}^{a/2}\frac{E_0}{a}\,e^{i\,ky\sin\theta}\,dy .

    Let α=ksin⁡θ=2πλsin⁡θ\alpha=k\sin\theta=\dfrac{2\pi}{\lambda}\sin\theta (a constant for a given angle). Then

    E=E0a∫−a/2a/2eiαy dy=E0a⋅eiαyiα∣−a/2a/2=E0a⋅eiαa/2−e−iαa/2iα.E=\frac{E_0}{a}\int_{-a/2}^{a/2} e^{i\alpha y}\,dy=\frac{E_0}{a}\cdot\frac{e^{i\alpha y}}{i\alpha}\Bigg|_{-a/2}^{a/2}=\frac{E_0}{a}\cdot\frac{e^{i\alpha a/2}-e^{-i\alpha a/2}}{i\alpha}.

    (b) Using eix−e−ix=2isin⁡xe^{ix}-e^{-ix}=2i\sin x,

    E=E0a⋅2isin⁡(αa/2)iα=E0a⋅2sin⁡(αa/2)α=E0 sin⁡(αa/2)αa/2.E=\frac{E_0}{a}\cdot\frac{2i\sin(\alpha a/2)}{i\alpha}=\frac{E_0}{a}\cdot\frac{2\sin(\alpha a/2)}{\alpha}=E_0\,\frac{\sin(\alpha a/2)}{\alpha a/2}.

    Define β=αa=kasin⁡θ=2πaλsin⁡θ\beta=\alpha a=ka\sin\theta=\dfrac{2\pi a}{\lambda}\sin\theta, so αa/2=β/2\alpha a/2=\beta/2 and

    E=E0 sin⁡(β/2)β/2.E=E_0\,\frac{\sin(\beta/2)}{\beta/2}.

    This is real for our phase reference, so ∣E∣=E0 sin⁡(β/2)β/2|E|=E_0\,\dfrac{\sin(\beta/2)}{\beta/2} (up to sign). Since intensity ∝∣E∣2\propto|E|^2, dividing by the central value I0I_0 (where the ratio is 11),

    I=I0[sin⁡(β/2)β/2]2.I=I_0\left[\frac{\sin(\beta/2)}{\beta/2}\right]^2 .

    (c) Minima occur where E=0E=0 with the peak not also vanishing — that is where sin⁡(β/2)=0\sin(\beta/2)=0 but β/2≠0\beta/2\ne0, i.e. β2=mπ\dfrac{\beta}{2}=m\pi for nonzero integer mm. Then

    πaλsin⁡θ=mπ⟹asin⁡θ=mλ,\frac{\pi a}{\lambda}\sin\theta=m\pi\quad\Longrightarrow\quad a\sin\theta=m\lambda,

    the standard single-slit dark-fringe condition.

    As θ→0\theta\to0, β/2→0\beta/2\to0, and using lim⁡x→0sin⁡xx=1\displaystyle\lim_{x\to0}\frac{\sin x}{x}=1,

    lim⁡θ→0I=I0(1)2=I0,\lim_{\theta\to0}I=I_0(1)^2=I_0,

    so the pattern peaks at the center, as expected. ■\blacksquare