Refraction of a plane wave: proving Snell's law
Light slows down in a denser medium, so the wavefront turns. Huygens' construction gives sin i / sin r = v₁/v₂, which is Snell's law.
Proof of Snell's law (rarer to denser medium)
A plane wavefront AB falls at an angle i on the surface PP′. Light travels at speed v₁ in medium 1 and v₂ in medium 2, with v₂ < v₁.
- 1End A of the wavefront touches the surface first. End B must travel BC in medium 1 to reach the surface at C.
- 2Let this take a time τ. So BC = v₁τ.
- 3In the same time, the secondary wavelet from A spreads into medium 2 with radius AE = v₂τ.
- 4From C, draw a tangent CE to this wavelet. CE is the refracted wavefront, making angle r with the surface.
- 5In right triangle ABC (right angle at B): sin i = BC/AC = v₁τ/AC.
- 6In right triangle AEC (right angle at E): sin r = AE/AC = v₂τ/AC.
- 7Divide the two: sin i / sin r = v₁/v₂.
- 8Put v₁ = c/n₁ and v₂ = c/n₂: sin i / sin r = n₂/n₁, so n₁ sin i = n₂ sin r.
- 9★So, sin i / sin r is a constant for the two media: this is Snell's law. Since v₂ < v₁, r < i and the ray bends towards the normal.
★ key step
Speed, wavelength and frequency on refraction
The frequency of light is fixed by the source, so it does not change on refraction. In the same time, the wavefront covers v₁τ in medium 1 and v₂τ in medium 2. If BC is one wavelength λ₁, then AE is one wavelength λ₂. So λ₁/λ₂ = v₁/v₂. In a denser medium, light is slower and its wavelength is shorter. Colour depends on frequency, so light keeps its colour inside water or glass.
Into a denser medium vs into a rarer medium
How to draw the refraction diagram
- Draw a horizontal line PP′. Write medium 1 (v₁) above it and medium 2 (v₂) below it.
- Draw the incident wavefront AB above the surface, touching it at A. Mark angle i between AB and PP′.
- Draw incident rays at right angles to AB, reaching A and C. Write BC = v₁τ.
- With A as centre, draw an arc of radius v₂τ below the surface. Make it clearly shorter than BC for a denser medium.
- From C, draw a tangent CE to the arc; label it refracted wavefront. Mark angle r between CE and PP′.
- Draw refracted rays at right angles to CE, and dashed normals at A and C.
Worked example: light entering glass
Light of wavelength 600 nm in air enters glass of refractive index 1.5. Find (a) its frequency, (b) its speed in glass, (c) its wavelength in glass. (c = 3 × 10⁸ m/s)
- Given: λ = 600 nm = 6 × 10⁻⁷ m, n = 1.5.
- (a) f = c/λ = (3 × 10⁸ m/s) ÷ (6 × 10⁻⁷ m) = 5 × 10¹⁴ Hz.
- (b) v = c/n = (3 × 10⁸ m/s) ÷ 1.5 = 2 × 10⁸ m/s.
- (c) λ′ = λ/n = 600 nm ÷ 1.5 = 400 nm.
- Check: v/λ′ = (2 × 10⁸ m/s) ÷ (4 × 10⁻⁷ m) = 5 × 10¹⁴ Hz, the same frequency as in air.
(a) 5 × 10¹⁴ Hz; (b) 2 × 10⁸ m/s; (c) 400 nm. The frequency does not change.
Worked example: angle of refraction in water
Light in air falls on water (n = 4/3) at an angle of incidence of 53°. Find the angle of refraction and the speed of light in water. (Take sin 53° = 0.8 and sin 37° = 0.6; c = 3 × 10⁸ m/s.)
- Snell's law: n₁ sin i = n₂ sin r, with n₁ = 1 for air.
- 1 × sin 53° = (4/3) × sin r.
- sin r = 0.8 × 3/4 = 0.6, so r = 37°.
- Speed in water: v = c/n = (3 × 10⁸ m/s) ÷ (4/3) = 2.25 × 10⁸ m/s.
r = 37°; v = 2.25 × 10⁸ m/s
A coin at the bottom of a bucket of water looks raised, because light from it bends away from the normal as it leaves the water. The optical fibres that carry internet across India work by total internal reflection, which the same wavefront picture explains.
3 marks: “Using Huygens' principle, verify Snell's law of refraction for a plane wave going from a rarer to a denser medium.” Diagram; BC = v₁τ; AE = v₂τ; tangent CE is the refracted wavefront; sin i = v₁τ/AC and sin r = v₂τ/AC; so sin i / sin r = v₁/v₂ = n₂/n₁; the ray bends towards the normal.
2 marks: “When light passes from air into glass, which of these change: frequency, wavelength, speed? Give a reason.” Speed and wavelength both decrease by the factor n. Frequency stays the same, because it is fixed by the source.
3 marks: “Light of wavelength 500 nm in air enters a medium of refractive index 1.25. Find its speed, wavelength and frequency in the medium.” v = (3 × 10⁸) ÷ 1.25 = 2.4 × 10⁸ m/s; λ′ = 500 ÷ 1.25 = 400 nm; f = (3 × 10⁸) ÷ (5 × 10⁻⁷) = 6 × 10¹⁴ Hz, unchanged.
Speed and wavelength shrink by n; frequency never changes. A slower medium gives a smaller wavelet, so the ray bends towards the normal.