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NSWPhysicsSyllabus dot point

Inquiry Question 1: What is light?

Analyse the wave model of light using Young's double-slit experiment, single-slit diffraction and polarisation, and apply Malus's law I = I_0 cos^2 theta to polarised light

A focused answer to the HSC Physics Module 7 dot point on the wave model of light. Young's double-slit interference with d sin theta = m lambda, single-slit diffraction, polarisation as evidence light is transverse, and quantitative use of Malus's law.

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  1. What this dot point is asking
  2. The answer
  3. Examples in context
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What this dot point is asking

NESA wants you to use the wave model of light to explain interference, diffraction and polarisation. You should be able to derive and apply the double-slit fringe condition, describe what a single-slit diffraction pattern looks like, explain polarisation as evidence that light is transverse, and use Malus's law quantitatively.

The answer

Why the wave model

Newton's particle (corpuscular) picture of light explained reflection and refraction but failed to predict diffraction and interference. By 1801 Thomas Young's double-slit experiment demonstrated that light produces interference fringes, which only waves can do. The wave model dominated nineteenth-century optics and motivated Maxwell's identification of light as an EM wave.

Young's double-slit experiment

Young's double slit experiment Coherent light from the left passes through two narrow slits separated by d in a barrier. Spherical waves emerge from each slit and overlap, producing alternating bright and dark fringes on a screen at distance L. Bright fringes are evenly spaced at delta y equals lambda L over d. light d screen L Bright fringes at d sin θ = mλ; fringe spacing Δy = λL ⁄ d.

Monochromatic, coherent light passing through two narrow slits separated by dd produces alternating bright and dark fringes on a screen at distance LL. Bright fringes occur where the path difference equals a whole number of wavelengths:

dsinθ=mλ,m=0,±1,±2,d \sin \theta = m \lambda, \quad m = 0, \pm 1, \pm 2, \dots

Dark fringes (destructive interference) occur where path difference is a half-odd integer:

dsinθ=(m+12)λd \sin \theta = (m + \tfrac{1}{2}) \lambda

For small angles, sinθtanθ=y/L\sin \theta \approx \tan \theta = y / L, so the bright-fringe positions on the screen are:

ym=mλLdy_m = \frac{m \lambda L}{d}

and the fringe spacing is:

Δy=λLd\Delta y = \frac{\lambda L}{d}

Three predictions of the wave model the experiment confirms:

  1. Increasing λ\lambda widens the fringes (red fringes wider than blue).
  2. Increasing dd narrows the fringes.
  3. Increasing LL widens the fringes.

Coherence (a fixed phase relationship between the two slits) is necessary, which is why a single source illuminates both slits.

Single-slit diffraction

A single slit of width aa produces a broader pattern with a wide central maximum and narrow, rapidly weakening side maxima. The dark fringes occur where:

asinθ=mλ,m=±1,±2,a \sin \theta = m \lambda, \quad m = \pm 1, \pm 2, \dots

The central maximum spans the angular range sinθ<λ/a|\sin \theta| < \lambda / a, twice the width of each side maximum.

In practice, the double-slit pattern is the product of two factors:

  • A double-slit interference pattern (equally spaced fringes from the two-slit geometry).
  • A single-slit diffraction envelope (each slit individually diffracts, modulating intensity).

Missing orders appear when a double-slit interference maximum coincides with a single-slit minimum.

Polarisation

Light is a transverse EM wave: E\vec{E} and B\vec{B} are perpendicular to the direction of propagation. Unpolarised light contains E\vec{E} vibrating in all directions perpendicular to the wave; a polarising filter passes only the component along its transmission axis.

Key observations only the transverse-wave model explains:

  • A polarising filter reduces unpolarised light to half its intensity (each direction averages to one component).
  • Two filters crossed at 9090^\circ transmit zero intensity.
  • Reflection off a non-metallic surface at Brewster's angle gives strongly polarised reflected light.

Longitudinal waves (such as sound) cannot be polarised, so polarisation is direct evidence that light is transverse.

Malus's law

If polarised light of intensity I0I_0 encounters a second polariser whose transmission axis makes angle θ\theta with the first:

I=I0cos2θ\boxed{I = I_0 \cos^2 \theta}

This follows from the projection E=E0cosθE = E_0 \cos \theta of the electric field onto the new axis, then squaring (intensity is proportional to E2E^2).

For unpolarised input, the first polariser halves the intensity, then any subsequent polariser follows Malus's law from there.

Worked example: two polarisers

Unpolarised light at 120120 W m2^{-2} enters two polarisers whose axes are at 4545^\circ to each other.

After polariser 1: I1=I0/2=60I_1 = I_0 / 2 = 60 W m2^{-2}.

After polariser 2: I2=I1cos245=60×0.5=30I_2 = I_1 \cos^2 45^\circ = 60 \times 0.5 = 30 W m2^{-2}.

If the second polariser is rotated to 9090^\circ, transmitted intensity drops to zero (cos290=0\cos^2 90^\circ = 0).

Examples in context

Example 1. Young's double-slit at a Sydney high-school physics lab. A laser of λ=633 nm\lambda = 633 \text{ nm} illuminates two slits separated by d=0.20 mmd = 0.20 \text{ mm}, projecting fringes on a screen L=2.50 mL = 2.50 \text{ m} away. Fringe spacing is Δy=λL/d=6.33×107×2.50/2.0×104=7.91×103 m=7.91 mm\Delta y = \lambda L / d = 6.33 \times 10^{-7} \times 2.50 / 2.0 \times 10^{-4} = 7.91 \times 10^{-3} \text{ m} = 7.91 \text{ mm}. The third-order bright fringe sits at angle sinθ=3λ/d=9.5×103\sin\theta = 3 \lambda / d = 9.5 \times 10^{-3}, so θ0.54\theta \approx 0.54^{\circ}. Sharp, evenly-spaced fringes confirm light is wavelike. Particle theory predicts only two bright bands directly behind each slit.

Example 2. Polarising filters on Bondi Beach photographers. Sunlight reflecting off the wet sand is partially polarised horizontally. A photographer rotates a polarising filter; when its transmission axis is vertical, Malus's law gives transmitted intensity I=I0cos290=0I = I_0 \cos^2 90^{\circ} = 0 for the horizontally-polarised glare, but I0/2I_0 / 2 for unpolarised sky-light passing through (averaged over all angles). Net effect: glare drops sharply while the blue sky stays bright. The fact that an EM wave's electric field is transverse means polarisation can do this; sound waves (longitudinal) cannot be polarised at all.

Try this

Q1. Distinguish between constructive and destructive interference in terms of path difference. [2 marks]

  • Cue. Constructive: Δx=mλ\Delta x = m\lambda (in phase). Destructive: Δx=(m+12)λ\Delta x = (m + \tfrac{1}{2})\lambda (anti-phase).

Q2. Two slits separated by 0.10 mm0.10 \text{ mm} are illuminated by light of λ=550 nm\lambda = 550 \text{ nm}. Calculate the angle to the second-order maximum. [2 marks]

  • Cue. dsinθ=mλd \sin\theta = m\lambda, so sinθ=2×5.5×107/1.0×104=0.011\sin\theta = 2 \times 5.5 \times 10^{-7} / 1.0 \times 10^{-4} = 0.011; θ=0.63\theta = 0.63^{\circ}.

Q3. Light is plane-polarised before passing through a second polariser. (a) State Malus's law. (b) If the analyser axis is at 6060^{\circ} to the polarisation direction, find the fraction of intensity transmitted. (c) Explain why polarisation provides evidence that light is a transverse wave. [1+2+3 marks]

  • Cue. (a) I=I0cos2θI = I_0 \cos^2\theta. (b) cos260=0.25\cos^2 60^{\circ} = 0.25. (c) Only transverse waves have a perpendicular electric-field direction that can be selectively transmitted; longitudinal waves (sound) cannot be polarised.

Exam-style practice questions

Practice questions written in the style of NESA exam questions on this dot point, with worked answer explainers. The year tag is the paper they imitate, not the source.

2021 HSC5 marksIn a Young's double-slit experiment, two slits 0.25 mm apart are illuminated with monochromatic light of wavelength 590 nm. The screen sits 1.8 m from the slits. Calculate the fringe spacing on the screen, and explain why a single-slit pattern would not show the same equally spaced bright fringes.
Show worked answer →

Fringe spacing for small angles:

Δy=λL/d=(5.90×107)(1.8)/(2.5×104)=4.25×103\Delta y = \lambda L / d = (5.90 \times 10^{-7})(1.8) / (2.5 \times 10^{-4}) = 4.25 \times 10^{-3} m =4.25= 4.25 mm.

Why a single slit looks different: a single slit produces a diffraction pattern from interference of light from the continuous range of points across the slit width. The central maximum is twice as wide as the side maxima, and side maxima fall off rapidly in intensity (envelope (sinα/α)2\propto (\sin \alpha / \alpha)^2). A double slit gives equally spaced narrow fringes from path-difference interference between the two slits, modulated by the single-slit envelope of each individual slit. So the equally spaced bright fringes come only when there are at least two coherent sources separated by a fixed distance dd.

Markers reward correct fringe-spacing formula and value, plus a clear contrast between two-source interference (equal spacing) and single-slit diffraction (broad central peak with rapidly weakening side peaks).

2018 HSC3 marksUnpolarised light of intensity 80 W m^-2 passes through two polarising filters whose transmission axes are at 30 degrees to each other. Calculate the intensity transmitted by the second filter, and state what would happen if a third filter were inserted between them at 60 degrees to the first.
Show worked answer →

After the first filter, unpolarised light is reduced to half its intensity (only one polarisation component passes):

I1=I0/2=80/2=40I_1 = I_0 / 2 = 80 / 2 = 40 W m2^{-2}.

Through the second filter (Malus's law with θ=30\theta = 30^\circ):

I2=I1cos230=40×(0.866)2=40×0.75=30I_2 = I_1 \cos^2 30^\circ = 40 \times (0.866)^2 = 40 \times 0.75 = 30 W m2^{-2}.

With a third filter inserted at 6060^\circ to the first (so 3030^\circ to the second on the entry side, and 3030^\circ to the original second filter on the exit side):

After the third filter: I1cos260=40×0.25=10I_1 \cos^2 60^\circ = 40 \times 0.25 = 10 W m2^{-2}.

After the original second filter (now 3030^\circ from the third): 10×cos230=10×0.75=7.510 \times \cos^2 30^\circ = 10 \times 0.75 = 7.5 W m2^{-2}.

Surprisingly, inserting an extra filter increases the final intensity from 00 when the original two are crossed at 9090^\circ, and changes the answer here too. Markers reward the half-intensity step, correct application of Malus's law, and recognition that polarisation order matters.

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