Module III: Interference in Thin Films - Question Solutions
Question 1: Thin Film Appears Black in Reflected Light
When light is incident on a very thin film (thickness t → 0), two reflected rays are produced:
- Ray R₁: Reflected from the top surface (air-film interface)
- Ray R₂: Reflected from the bottom surface (film-substrate interface)
For a thin film (n > 1) on a substrate:
- R₁: Reflects at air-film interface (going from lower n to higher n) → Phase change of π
- R₂: Reflects at film-substrate interface (depends on substrate, typically no additional phase change relative to R₁)
For a film of thickness t, the path difference between R₁ and R₂ is:
When t → 0 (excessively thin film):
Including the phase change of λ/2 (equivalent to π phase shift):
A path difference of λ/2 corresponds to destructive interference.
When the two reflected rays are exactly out of phase (180° or λ/2 path difference), they cancel each other completely.
- The geometric path difference (2μt cos r) is nearly zero
- The only path difference comes from the π phase change at the air-film interface
- This λ/2 effective path difference causes complete destructive interference
- No light is reflected, making the film appear black
Practical Example: This is why soap bubbles appear black just before they burst - at that point, the film becomes extremely thin.
Question 2: Conditions for Maxima and Minima in Thin Films
Consider a thin film of uniform thickness t and refractive index μ. A ray of light incident at angle i is partially reflected (R₁) and partially refracted at angle r. The refracted ray reflects from the bottom surface, giving ray R₂.
Step 1: The path traveled by ray R₂ inside the film is BC + CD.
From geometry: BC = CD = t/cos r
Step 2: Optical path in film = μ(BC + CD) = μ × 2t/cos r = 2μt/cos r
Step 3: Path traveled by R₁ in air = BN (where N is on the extended R₁ path)
BN = BD × sin i, and BD = 2t × tan r
Therefore, BN = 2t × tan r × sin i
Step 4: Using Snell's law: sin i = μ sin r
BN = 2t × tan r × μ sin r = 2μt × sin²r/cos r
Step 5: Path difference:
Ray R₁ undergoes a phase change of π (equivalent to λ/2 path difference) upon reflection from denser medium.
For bright fringes, effective path difference = nλ (where n = 0, 1, 2, ...)
Or: 2μt cos r = (n - ½)λ, where n = 1, 2, 3, ...
For dark fringes, effective path difference = (2n + 1)λ/2
where n = 0, 1, 2, 3, ...
| Condition | Reflected Light | Transmitted Light |
|---|---|---|
| Maxima (Bright) | 2μt cos r = (2n-1)λ/2 | 2μt cos r = nλ |
| Minima (Dark) | 2μt cos r = nλ | 2μt cos r = (2n-1)λ/2 |
Question 3: Newton's Rings - Refractive Index Determination
Newton's rings are formed due to interference between light reflected from the lower surface of the plano-convex lens and the upper surface of the flat glass plate. The air film between them has varying thickness, creating concentric circular interference fringes.
For the nᵗʰ dark ring with air between lens and plate:
When a liquid of refractive index μ is placed between the lens and plate:
- Does not require knowledge of wavelength λ or radius R
- Only ratio of squared diameters is needed
- Can be used for transparent liquids
- High accuracy with proper measurements
Question 4: Newton's Rings Numerical - Radius of Curvature
- Diameter of 5ᵗʰ dark ring, D₅ = 0.336 cm = 0.336 × 10⁻² m
- Diameter of 15ᵗʰ dark ring, D₁₅ = 0.590 cm = 0.590 × 10⁻² m
- Wavelength, λ = 5890 Å = 5890 × 10⁻¹⁰ m = 5.89 × 10⁻⁷ m
- n = 5, m = 15
Therefore:
Calculate D₁₅² - D₅²:
Calculate 4(m - n)λ:
Calculate R:
Question 5: Newton's Rings with Liquid - Numerical
- Refractive index of liquid, μ = 1.33
- Diameter of 9ᵗʰ dark ring, D₉ = 0.58 cm = 0.58 × 10⁻² m
- Wavelength, λ = 6000 Å = 6000 × 10⁻¹⁰ m = 6 × 10⁻⁷ m
- n = 9
Solving for R:
Calculate Dₙ²:
Calculate 4nλ:
Calculate R: