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UNIT SYLLABUS

C.3 Wave phenomena

SL/HL 5 hours SL + 6 hours HL
This is where waves do things particles never could. At boundaries they reflect and refract (Snell's law, total internal reflection — the physics of optical fibres); around obstacles they diffract; and when two coherent waves meet they interfere, adding crest-on-crest or cancelling crest-on-trough. Young's double-slit experiment turns that superposition into a measuring instrument fine enough to determine the wavelength of light with a ruler. HL sharpens the picture with single-slit diffraction — whose envelope modulates the double-slit pattern — and diffraction gratings, which power every spectrometer that has ever decoded starlight.

Guiding Questions

  • ? How do waves behave at boundaries between different media?
  • ? What happens when two waves occupy the same region of space at the same time?

What the IB expects you to master

  • Describe two- and three-dimensional waves using wavefronts and rays.
  • Analyse reflection, refraction and transmission at boundaries, including wavefront–ray diagrams.
  • Apply Snell's law n1n2=sinθ2sinθ1=v2v1\frac{n_1}{n_2} = \frac{\sin\theta_2}{\sin\theta_1} = \frac{v_2}{v_1}, the critical angle, and total internal reflection.
  • Describe diffraction around bodies and through apertures, and its dependence on the ratio λ/b\lambda/b.
  • Explain superposition of waves and pulses, and the need for coherent sources in double-source interference.
  • Use the interference conditions: constructive at path difference nλn\lambda, destructive at (n+12)λ(n+\frac{1}{2})\lambda.
  • Apply Young's double-slit equation s=λDds = \frac{\lambda D}{d} for fringe spacing.
  • HL: use single-slit diffraction (θ=λ/b\theta = \lambda/b for the first minimum) and explain how it modulates the double-slit pattern.
  • HL: analyse multiple slits and diffraction gratings with nλ=dsinθn\lambda = d\sin\theta.

1 Key Formulas

Snell's law
n1n2=sinθ2sinθ1=v2v1\frac{n_{1}}{n_{2}} = \frac{\sin\theta_{2}}{\sin\theta_{1}} = \frac{v_{2}}{v_{1}}
Refractive index
n=cvn = \frac{c}{v}
Constructive interference
path difference=nλ\text{path difference} = n\lambda
Destructive interference
path difference=(n+12)λ\text{path difference} = \left(n + \tfrac{1}{2}\right)\lambda
Double-slit fringe spacing
s=λDds = \frac{\lambda D}{d}
Single-slit first minimum (HL)
θ=λb\theta = \frac{\lambda}{b}
Diffraction grating maxima (HL)
nλ=dsinθn\lambda = d\sin\theta

2 Exam Preparation & Topic Explanations

Interference calculations that always land

Every interference question reduces to path difference. Constructive: whole wavelengths. Destructive: odd half-wavelengths. State that first, then substitute the geometry — double slit, grating, or thin film.

For gratings, remember maxima are sharp and bright (many slits reinforce), and always check nλdn\lambda \le d to count visible orders.

Pro Exam Strategy
  • Snell's law in the IB data booklet form has the indices inverted relative to many textbooks: n1sinθ1=n2sinθ2n_1\sin\theta_1 = n_2\sin\theta_2 is safest to work from.

  • Angles are measured from the NORMAL, never the surface.

  • Grating question: convert "lines per mm" to slit spacing dd in metres first, before anything else.

  • HL: missing orders occur when a double-slit maximum coincides with a single-slit minimum — the envelope kills it.

3 MCQ Practice

Q1. Light travels from glass (n=1.5n = 1.5) towards air. The critical angle is approximately:

  • 30°
  • 42°
  • 48°
  • 60°

Q2. In a double-slit experiment, the slit separation is doubled and the screen distance halved. The fringe spacing becomes:

  • Four times larger
  • Unchanged
  • A quarter of the original
  • Half the original

Q3. Sound diffracts around a doorway much more than light does because:

  • Sound travels more slowly than light
  • Sound is longitudinal and light is transverse
  • Sound's wavelength is comparable to the width of the doorway
  • Sound has more energy than light

4 Short Answer Questions

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