Interference and Diffraction

Young's double slit, single slit diffraction, diffraction grating, thin film interference

🌈 Interference and Diffraction

Wave Nature of Light

Light exhibits wave properties:

  • Interference (constructive and destructive)
  • Diffraction (bending around obstacles)
  • Polarization

These prove light is a wave!


Young's Double Slit

Two narrow slits illuminated by coherent light:

Path difference determines interference:

Bright fringes (constructive): dsinθ=mλd \sin\theta = m\lambda

Dark fringes (destructive): dsinθ=(m+12)λd \sin\theta = \left(m + \frac{1}{2}\right)\lambda

where:

  • d = slit separation
  • θ = angle from center
  • m = order (0, ±1, ±2, ...)
  • λ = wavelength

Small angle approximation (θ << 1 rad): sinθtanθyL\sin\theta \approx \tan\theta \approx \frac{y}{L}

Fringe spacing on screen: Δy=λLd\Delta y = \frac{\lambda L}{d}

where L = distance to screen

💡 Key: Smaller slit spacing d → larger fringe spacing Δy!


Conditions for Interference

  1. Coherent sources: Constant phase relationship
  2. Monochromatic: Single wavelength (or narrow range)
  3. Similar amplitudes: For clear pattern

Laser light is ideal!


Single Slit Diffraction

Single wide slit creates diffraction pattern:

Dark fringes: asinθ=mλa \sin\theta = m\lambda

where:

  • a = slit width
  • m = ±1, ±2, ... (NOT zero!)

Central maximum: Brightest, twice as wide as other maxima

Width of central max: w=2λLaw = \frac{2\lambda L}{a}

💡 Key: Narrower slit a → wider central maximum!

Difference from double slit:

  • Double slit: Narrow bright fringes (interference)
  • Single slit: Wide central max, dimmer side maxima (diffraction)

Diffraction Grating

Many equally-spaced slits (100s to 1000s per mm):

Bright fringes (very sharp!): dsinθ=mλd \sin\theta = m\lambda

where d = spacing between slits

Advantages:

  • Very sharp, bright lines
  • Separates wavelengths well (spectroscopy!)
  • Higher orders (larger m) more spread out

Dispersion: Different λ at different angles

  • Red: longer λ, larger θ
  • Violet: shorter λ, smaller θ

Resolving power: R=mNR = mN (N = number of slits)


Thin Film Interference

Light reflects from top and bottom surfaces of thin film:

Phase change on reflection:

  • Fast to slow (n_low to n_high): 180° = λ/2 shift
  • Slow to fast: No phase change

Constructive interference:

  • If ONE reflection has phase change: 2t=(m+12)λn2t = \left(m + \frac{1}{2}\right)\lambda_n

  • If ZERO or TWO reflections have phase change: 2t=mλn2t = m\lambda_n

where:

  • t = film thickness
  • λn=λ/n\lambda_n = \lambda/n = wavelength in film

Destructive is opposite!

Applications:

  • Soap bubbles (swirling colors)
  • Oil slicks on water
  • Anti-reflection coatings (destructive for reflection)

Polarization

Light wave with E field oscillating in one plane only.

UnpolarizedPolarized: Use polarizer (absorbs one component)

Malus's Law: Intensity through second polarizer I=I0cos2θI = I_0 \cos^2\theta

where θ = angle between polarizers

Crossed polarizers (θ = 90°): No light passes!

Ways to polarize:

  1. Polarizing filter
  2. Reflection (Brewster's angle)
  3. Scattering (why sky is blue and polarized!)

Rayleigh Criterion (Resolution)

Two point sources barely resolved when:

θmin=1.22λD\theta_{min} = 1.22\frac{\lambda}{D}

where D = aperture diameter

Smaller θ_min → better resolution

  • Larger aperture (telescope!) → better
  • Shorter wavelength (blue light) → better

Problem-Solving Strategy

Double Slit:

  1. Bright: dsinθ=mλd \sin\theta = m\lambda
  2. Use small angle: sinθy/L\sin\theta \approx y/L
  3. Fringe spacing: Δy=λL/d\Delta y = \lambda L/d

Single Slit:

  1. Dark: asinθ=mλa \sin\theta = m\lambda (m ≠ 0)
  2. Central max width: w=2λL/aw = 2\lambda L/a

Thin Film:

  1. Count phase changes (reflections)
  2. Use λn=λ/n\lambda_n = \lambda/n in film
  3. Path difference = 2t
  4. Add/subtract λ/2 for phase changes

Common Mistakes

❌ Confusing d (slit separation) with a (slit width) ❌ Using m = 0 for single slit dark fringe (m starts at ±1!) ❌ Forgetting λ_n = λ/n in thin films ❌ Not accounting for phase change on reflection ❌ Wrong units (nm vs m, degrees vs radians) ❌ Thinking larger slit spacing → larger fringe spacing (opposite!)

📚 Practice Problems

1Problem 1hard

Question:

In a double-slit experiment, light with wavelength 600 nm passes through slits separated by 0.10 mm. A screen is 2.0 m away. (a) What is the distance between adjacent bright fringes? (b) What is the angle to the third-order bright fringe?

💡 Show Solution

Solution:

Given: λ = 600 nm = 6.0 × 10⁻⁷ m, d = 0.10 mm = 1.0 × 10⁻⁴ m, L = 2.0 m

(a) Distance between bright fringes: For small angles: Δy = λL/d Δy = (6.0 × 10⁻⁷)(2.0)/(1.0 × 10⁻⁴) Δy = (12 × 10⁻⁷)/(1.0 × 10⁻⁴) Δy = 1.2 × 10⁻² m or 1.2 cm

(b) Angle to third bright fringe (m = 3): d sin θ = mλ sin θ = mλ/d = 3(6.0 × 10⁻⁷)/(1.0 × 10⁻⁴) sin θ = (18 × 10⁻⁷)/(1.0 × 10⁻⁴) = 0.018 θ = 1.03° or 1.0°

Very small angle (small angle approximation valid).

2Problem 2medium

Question:

Light of wavelength 500 nm passes through a single slit of width 0.050 mm. (a) What is the angular width of the central bright fringe? (b) If the screen is 1.5 m away, what is the linear width of the central maximum?

💡 Show Solution

Solution:

Given: λ = 500 nm = 5.0 × 10⁻⁷ m, a = 0.050 mm = 5.0 × 10⁻⁵ m, L = 1.5 m

(a) Angular width of central maximum: First minimum occurs at: a sin θ = λ sin θ = λ/a = (5.0 × 10⁻⁷)/(5.0 × 10⁻⁵) = 0.010 θ = 0.573° (to first minimum on one side)

Angular width = 2θ = 1.15° or 1.1° (center to both first minima)

(b) Linear width on screen: y = L tan θ ≈ L sin θ (small angle) y = (1.5)(0.010) = 0.015 m (to first minimum)

Total width = 2y = 3.0 cm (or 0.030 m)

Central maximum is twice as wide as other maxima in single-slit diffraction.

3Problem 3easy

Question:

In a double slit experiment with 550 nm light, slits are 0.20 mm apart, and screen is 2.0 m away. What is the spacing between bright fringes?

💡 Show Solution

Given:

  • Wavelength: λ=550\lambda = 550 nm =5.5×107= 5.5 \times 10^{-7} m
  • Slit separation: d=0.20d = 0.20 mm =2.0×104= 2.0 \times 10^{-4} m
  • Screen distance: L=2.0L = 2.0 m

Solution:

Fringe spacing: Δy=λLd=(5.5×107)(2.0)2.0×104\Delta y = \frac{\lambda L}{d} = \frac{(5.5 \times 10^{-7})(2.0)}{2.0 \times 10^{-4}} Δy=1.1×1062.0×104=5.5×103 m\Delta y = \frac{1.1 \times 10^{-6}}{2.0 \times 10^{-4}} = 5.5 \times 10^{-3} \text{ m} Δy=5.5 mm\Delta y = 5.5 \text{ mm}

Answer: Fringe spacing = 5.5 mm

Bright fringes are 5.5 mm apart on the screen.

4Problem 4easy

Question:

In a double slit experiment with 550 nm light, slits are 0.20 mm apart, and screen is 2.0 m away. What is the spacing between bright fringes?

💡 Show Solution

Given:

  • Wavelength: λ=550\lambda = 550 nm =5.5×107= 5.5 \times 10^{-7} m
  • Slit separation: d=0.20d = 0.20 mm =2.0×104= 2.0 \times 10^{-4} m
  • Screen distance: L=2.0L = 2.0 m

Solution:

Fringe spacing: Δy=λLd=(5.5×107)(2.0)2.0×104\Delta y = \frac{\lambda L}{d} = \frac{(5.5 \times 10^{-7})(2.0)}{2.0 \times 10^{-4}} Δy=1.1×1062.0×104=5.5×103 m\Delta y = \frac{1.1 \times 10^{-6}}{2.0 \times 10^{-4}} = 5.5 \times 10^{-3} \text{ m} Δy=5.5 mm\Delta y = 5.5 \text{ mm}

Answer: Fringe spacing = 5.5 mm

Bright fringes are 5.5 mm apart on the screen.

5Problem 5medium

Question:

A single slit of width 0.050 mm produces a diffraction pattern with 600 nm light on a screen 1.5 m away. What is the width of the central bright maximum?

💡 Show Solution

Given:

  • Slit width: a=0.050a = 0.050 mm =5.0×105= 5.0 \times 10^{-5} m
  • Wavelength: λ=600\lambda = 600 nm =6.0×107= 6.0 \times 10^{-7} m
  • Screen distance: L=1.5L = 1.5 m

Solution:

Width of central maximum: w=2λLa=2(6.0×107)(1.5)5.0×105w = \frac{2\lambda L}{a} = \frac{2(6.0 \times 10^{-7})(1.5)}{5.0 \times 10^{-5}} w=1.8×1065.0×105=0.036 mw = \frac{1.8 \times 10^{-6}}{5.0 \times 10^{-5}} = 0.036 \text{ m} w=36 mm=3.6 cmw = 36 \text{ mm} = 3.6 \text{ cm}

Answer: Central maximum width = 3.6 cm

This is the distance between the first dark fringes on either side of center.

6Problem 6medium

Question:

A single slit of width 0.050 mm produces a diffraction pattern with 600 nm light on a screen 1.5 m away. What is the width of the central bright maximum?

💡 Show Solution

Given:

  • Slit width: a=0.050a = 0.050 mm =5.0×105= 5.0 \times 10^{-5} m
  • Wavelength: λ=600\lambda = 600 nm =6.0×107= 6.0 \times 10^{-7} m
  • Screen distance: L=1.5L = 1.5 m

Solution:

Width of central maximum: w=2λLa=2(6.0×107)(1.5)5.0×105w = \frac{2\lambda L}{a} = \frac{2(6.0 \times 10^{-7})(1.5)}{5.0 \times 10^{-5}} w=1.8×1065.0×105=0.036 mw = \frac{1.8 \times 10^{-6}}{5.0 \times 10^{-5}} = 0.036 \text{ m} w=36 mm=3.6 cmw = 36 \text{ mm} = 3.6 \text{ cm}

Answer: Central maximum width = 3.6 cm

This is the distance between the first dark fringes on either side of center.

7Problem 7hard

Question:

A soap film (n = 1.33) is 450 nm thick. What wavelength of visible light (in air) is most strongly reflected? Assume normal incidence.

💡 Show Solution

Given:

  • Film index: n=1.33n = 1.33
  • Thickness: t=450t = 450 nm
  • Air on both sides (n = 1.00)

Solution:

Step 1: Count phase changes.

  • Top surface: air (1.00) → film (1.33) = phase change (λ/2)
  • Bottom surface: film (1.33) → air (1.00) = no phase change

One phase change total

Step 2: Constructive interference (for ONE phase change): 2t=(m+12)λn=(m+12)λn2t = \left(m + \frac{1}{2}\right)\lambda_n = \left(m + \frac{1}{2}\right)\frac{\lambda}{n} λ=2tnm+1/2\lambda = \frac{2tn}{m + 1/2}

Step 3: Try m = 0, 1, 2... to find visible wavelength (400-700 nm)

m=0m = 0: λ=2(450)(1.33)0.5=2394 nm\lambda = \frac{2(450)(1.33)}{0.5} = 2394 \text{ nm} (infrared, too long)

m=1m = 1: λ=2(450)(1.33)1.5=798 nm\lambda = \frac{2(450)(1.33)}{1.5} = 798 \text{ nm} (infrared, too long)

m=2m = 2: λ=2(450)(1.33)2.5=479 nm\lambda = \frac{2(450)(1.33)}{2.5} = 479 \text{ nm} (blue-green, visible!) ✓

Answer: λ = 479 nm (blue-green light)

This is why soap bubbles appear colored!

8Problem 8hard

Question:

A soap film (n = 1.33) is 450 nm thick. What wavelength of visible light (in air) is most strongly reflected? Assume normal incidence.

💡 Show Solution

Given:

  • Film index: n=1.33n = 1.33
  • Thickness: t=450t = 450 nm
  • Air on both sides (n = 1.00)

Solution:

Step 1: Count phase changes.

  • Top surface: air (1.00) → film (1.33) = phase change (λ/2)
  • Bottom surface: film (1.33) → air (1.00) = no phase change

One phase change total

Step 2: Constructive interference (for ONE phase change): 2t=(m+12)λn=(m+12)λn2t = \left(m + \frac{1}{2}\right)\lambda_n = \left(m + \frac{1}{2}\right)\frac{\lambda}{n} λ=2tnm+1/2\lambda = \frac{2tn}{m + 1/2}

Step 3: Try m = 0, 1, 2... to find visible wavelength (400-700 nm)

m=0m = 0: λ=2(450)(1.33)0.5=2394 nm\lambda = \frac{2(450)(1.33)}{0.5} = 2394 \text{ nm} (infrared, too long)

m=1m = 1: λ=2(450)(1.33)1.5=798 nm\lambda = \frac{2(450)(1.33)}{1.5} = 798 \text{ nm} (infrared, too long)

m=2m = 2: λ=2(450)(1.33)2.5=479 nm\lambda = \frac{2(450)(1.33)}{2.5} = 479 \text{ nm} (blue-green, visible!) ✓

Answer: λ = 479 nm (blue-green light)

This is why soap bubbles appear colored!