Foundations
Sections 7.1, 7.2, 7.3
Reflection
Incident ray, reflected ray and normal lie in one plane.Refraction (Snell)
Incident ray, refracted ray and normal lie in one plane.How the theory of light evolved
| Theory | Who | Idea | Verdict |
|---|---|---|---|
| Corpuscular | Descartes (1636), Newton | Light = hard, elastic, massless particles. Elastic collisions explain reflection; medium attraction explains refraction. | Predicts vdenser > vrarer, which experiment contradicts. |
| Wave | Huygens (1668) | Light is a wave in a hypothetical medium, ether. Explains interference, diffraction, polarization, reflection, refraction. | Accepted. Gives vdenser < vrarer. Ether never found (Michelson–Morley); Einstein (1905) removed the need for it. |
| Dual | Early 20th century | Light shows wave nature or particle nature depending on the situation. Particle of light = photon. | Modern view. |
Light as an electromagnetic wave (7.3)
Light is a transverse electromagnetic wave. E and B are perpendicular to each other and to the direction of travel. It needs no medium, so it crosses vacuum.
Spectrum, increasing wavelength: γ-rays → X-rays → UV → Visible → IR → Microwaves → Radio. Visible light spans 400–700 nm; violet is shortest, red longest. Because n depends on wavelength, white light splits into a spectrum or rainbow (except at normal incidence).
Wavefronts and Huygens
Section 7.4
Primary source
Emits its own light: Sun, stars, flame, tube light, TV, firecrackers.Secondary source
Reflects or scatters light from elsewhere: Moon, planets, humans, plants. Most everyday sources are secondary.| Source | Wavefront | Rays |
|---|---|---|
| Point source | Spherical | Radiate out, ⟂ to the surface (diverging beam) |
| Far from source | Plane | Parallel, ⟂ to the wavefront (parallel beam) |
| Linear source | Cylindrical | ⟂ to the surface |
A plane wave is a wave with a plane wavefront. A ray is always perpendicular to the wavefront.
Reflection and Refraction
Sections 7.5, 7.6 · Both are long-answer derivations
Derive the law of reflection
- Plane wavefront AB hits mirror MN. At t = 0, A touches the mirror; B has not.
- B reaches C after time T, so BC = vT.
- Points from A to C become secondary sources one after another.
- At time T the wavelet from A has radius AE = vT, so AE = BC. The envelope is the reflected wavefront EC.
- Triangles ABC and AEC are right-angled, share hypotenuse AC and have AE = BC, so they are congruent.
- ∠ACE = ∠BAC = i. Since AE ⟂ CE and AP ⟂ AC, ∠PAE = ∠ACE = r.
- Therefore i = r. Incident ray, reflected ray and normal lie in one plane.
Derive Snell's law
- Wavefront AB meets boundary MN. Speeds are v₁ (medium 1) and v₂ (medium 2).
- B reaches C in time T: BC = v₁T. Meanwhile the wavelet from A travels AE = v₂T in medium 2.
- Envelope of wavelets = refracted wavefront CE.
- sin i = BC/AC = v₁T/AC and sin r = AE/AC = v₂T/AC.
- Divide: sin i / sin r = v₁/v₂.
- With v = c/n: v₁/v₂ = n₂/n₁.
- Hence n₁ sin i = n₂ sin r.
Rarer → denser
v drops, n rises, i > r. Ray bends towards the normal.Denser → rarer
Ray bends away from the normal.What changes when light enters a new medium?
| Speed v | Wavelength λ | Frequency ν |
|---|---|---|
| Changes | Changes | Unchanged |
Lateral inversion — the apparent interchange of right and left in a mirror image. Image size equals object size.
Lab: refraction calculator
Polarization
Section 7.7 · Proves light is a transverse wave
Unpolarized
E vibrates in all directions perpendicular to travel (Sun, bulb).Plane polarized
E restricted to one direction.Polarizer
Transmits E along one direction, blocks others. A polaroid is a plastic-sheet polarizer; the allowed direction is the polarizing axis.Why transverse only? A transverse wave has many possible oscillation directions to restrict. A longitudinal wave (sound) oscillates along travel, so there is nothing to restrict.
Plane of vibration contains E. Plane of polarization is perpendicular to it. Parallel axes (θ = 0°) pass all light; crossed axes (θ = 90°) pass none.
Malus' law
Lab: Malus' law
Brewster's law
Derive tan θB = n₂/n₁
- Snell: n₁ sin θB = n₂ sin θr
- θr = 90° − θB, so sin θr = cos θB
- n₁ sin θB = n₂ cos θB
- Divide by n₁ cos θB: tan θB = n₂/n₁
Example: air to n = 1.5 gives θB = tan⁻¹(1.5) = 56.31°. Polaroid sunglasses cut glare from non-metallic surfaces.
Scattering: sunlight hitting air molecules and dust changes direction; blue scatters most, so the sky is blue. Scattered light is partially polarized, and at a 90° scattering angle it is plane polarized.
Interference
Section 7.8 · Young first observed it for light in 1801
Young's double slit (D ≫ d)
Path difference
Bright fringe
yₙ = nλD / d
Dark fringe
yₙ = (n − ½)λD / d
Fringe width
| Path diff. | Phase diff. | Intensity | |
|---|---|---|---|
| Bright | nλ | 2nπ | 4I₀ |
| Dark | (n − ½)λ | (2n − 1)π | 0 |
With unequal amplitudes, Imax ∝ (E₁ + E₂)² and Imin ∝ (E₁ − E₂)², so dark fringes are not fully dark.
Lab: Young's double slit
Conditions for a steady pattern — C M A D N P
| Coherent sources | Monochromatic light | Equal Amplitudes |
| D ≫ d | Narrow slits | Same Polarization |
A constant non-zero phase difference between sources shifts the whole pattern but leaves fringe width unchanged.
Other ideas
Lloyd's mirror
Direct ray plus ray reflected at grazing incidence, which seems to come from a virtual source. Real + virtual source are coherent.Thin films
Soap bubbles and oil films: light reflected from the top surface interferes with light reflected from the bottom. Reflection from a denser boundary adds phase π (path λ/2).Optical path
Transparent plate on one slit
Diffraction
Section 7.9
| Fraunhofer (Far) | Fresnel (Near) |
|---|---|
| Very large distances; plane incident wavefront; lenses used | Smaller distances; cylindrical or spherical wavefront; no lens needed |
Single slit of width a (D ≫ a)
- Centre P₀: all paths equal, so a central bright maximum.
- Extreme-ray path difference is a sinθ. For the first minimum, halves of the slit cancel in pairs (λ/2 apart).
nth minimum
yₙ = nλD / a
Secondary maxima
Fringe width
Central maximum
Interference vs diffraction
| YDSE | Single slit | |
|---|---|---|
| Waves | Two coherent | Many, from one slit |
| Width | λD/d (d = slit separation) | λD/a (a = slit width) |
| Central fringe | Same width as others | Twice as wide |
| Brightness | Nearly equal | Centre brightest, others weaker |
Exam Toolkit
Revise here the night before
Definitions to write word-perfect
Formula sheet
| Topic | Formula |
|---|---|
| Refractive index | n = c/v |
| Snell's law | n₁ sin i = n₂ sin r |
| Wavelength in medium | λ = λ₀/n; λ₂ = λ₁n₁/n₂ |
| Wavelet radius | r = vT |
| Malus | I = I₀cos²θ; first polarizer I₀/2 |
| Brewster | tanθB = n₂/n₁ |
| YDSE | Δl = yd/D; W = λD/d; I = 4I₀cos²(φ/2) |
| Plate on slit | (n − 1)t |
| Single slit | a sinθ = nλ; W = λD/a; W_c = 2λD/a |