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light interference diffraction and polarization

Learning objectives

  • Outcome

    Calculate the positions of maxima and the fringe spacing in Young's double-slit experiment using Δy=λL/d\Delta y = \lambda L/d and dsin⁡θ=mλd\sin\theta = m\lambda.

  • Outcome

    Determine the angles of principal maxima for a diffraction grating and minima for a single slit using dsin⁡θ=mλd\sin\theta = m\lambda and asin⁡θ=mλa\sin\theta = m\lambda.

  • Outcome

    Apply Malus's law I=I0cos⁡2θI = I_0\cos^2\theta to calculate intensity after polarizers.

Understand the idea

Interference, Diffraction, and Polarization of Light

Text

Light is an electromagnetic wave, so wave laws apply to it: interference arises when coherent waves superpose, and diffraction arises when the wavefront is limited. In Young's experiment the path difference Δ=dsin⁡θ\Delta = d\sin\theta gives maxima when Δ=mλ\Delta = m\lambda and minima when Δ=(m+12)λ\Delta = (m+\tfrac12)\lambda. For a diffraction grating, the condition for principal maxima dsin⁡θ=mλd\sin\theta = m\lambda gives the angles at which different wavelengths are separated. Single-slit diffraction is described by minima asin⁡θ=mλa\sin\theta = m\lambda, where aa is the slit width. Polarization reveals the transverse nature of light waves: after a polarizer, the intensity obeys Malus's law I=I0cos⁡2θI = I_0\cos^2\theta if the incident light is linearly polarized. These phenomena share a common wave language: amplitude, phase difference, and projection of the electric-field vector.

Worked examples

Direct

Problem

In Young's experiment, light with wavelength λ=600\lambda = 600 nm falls on two slits separated by d=0.20d = 0.20 mm. The screen is placed at a distance L=2.0L = 2.0 m. Find the fringe spacing, that is, the distance between adjacent bright fringes.

Solution

The fringe spacing is the distance between adjacent maxima, so Δy=λL/d\Delta y = \lambda L/d. Substitute SI values: λ=600×10−9\lambda = 600\times10^{-9} m, d=0.20×10−3d = 0.20\times10^{-3} m, L=2.0L = 2.0 m. Then Δy=600×10−9⋅2.00.20×10−3=6.0×10−3.\Delta y = \frac{600\times10^{-9}\cdot 2.0}{0.20\times10^{-3}} = 6.0\times10^{-3}. Convert to millimeters: Δy=6.0\Delta y = 6.0 mm. This is the distance between adjacent bright fringes.

Application

Problem

Unpolarized light of intensity I0I_0 passes through two polarizers. The axis of the first is vertical, and the axis of the second makes an angle 60∘60^\circ with the vertical. Find the intensity of the light after the second polarizer.

Solution

The first polarizer reduces the intensity of unpolarized light by half: I1=I0/2I_1 = I_0/2. The second polarizer acts according to Malus's law: I2=I1cos⁡2θI_2 = I_1\cos^2\theta. For θ=60∘\theta = 60^\circ, I2=I02cos⁡260∘=I02(12)2=I08.I_2 = \frac{I_0}{2}\cos^2 60^\circ = \frac{I_0}{2}\left(\frac12\right)^2 = \frac{I_0}{8}. Answer: I0/8I_0/8.

Transfer

Problem

Linearly polarized light with wavelength λ=600\lambda = 600 nm illuminates two slits separated by d=0.15d = 0.15 mm. The screen is L=1.5L = 1.5 m from the slits. An analyzer is placed in front of the screen, and its axis makes an angle 30∘30^\circ with the polarization direction of the incident light. Find the distance from the central maximum to the first side maximum and the factor by which the intensity at this maximum is smaller than the intensity at the same maximum without the analyzer.

Solution

The position of the first side maximum is determined by interference: y1=λL/dy_1 = \lambda L/d. In SI units: λ=600×10−9\lambda = 600\times10^{-9} m, d=0.15×10−3d = 0.15\times10^{-3} m, L=1.5L = 1.5 m. Then y1=600×10−9⋅1.50.15×10−3=6.0×10−3.y_1 = \frac{600\times10^{-9}\cdot 1.5}{0.15\times10^{-3}} = 6.0\times10^{-3}. Thus y1=6.0y_1 = 6.0 mm. The analyzer does not shift the maxima because both slits produce light with the same polarization; it only attenuates the intensity according to Malus's law. For θ=30∘\theta = 30^\circ, the transmission factor is cos⁡230∘=(3/2)2=3/4\cos^2 30^\circ = (\sqrt{3}/2)^2 = 3/4. Therefore the intensity with the analyzer is 3/43/4 of the intensity without the analyzer, i.e. smaller by a factor of 4/34/3. Answer: 6.06.0 mm; smaller by a factor of 4/34/3.

Practice

Text

Carry out an independent investigation. Open the PhET simulation 'Wave Interference' (or a similar one) and select the light two-slit mode. Fix λ=600\lambda = 600 nm, d=0.20d = 0.20 mm, and vary LL from 1 to 3 m; record the positions of the first three maxima and test the formula Δy=λL/d\Delta y = \lambda L/d. Then switch to one slit and measure the angles of the minima, comparing them with asin⁡θ=mλa\sin\theta = m\lambda. For polarization, safely use two polarizing filters (for example, from sunglasses) and a laptop screen: rotating the second filter, verify that at angles 0∘,30∘,45∘,60∘,90∘0^\circ, 30^\circ, 45^\circ, 60^\circ, 90^\circ the brightness qualitatively follows I∝cos⁡2θI \propto \cos^2\theta. Do not look directly at the Sun and do not use powerful sources; if in doubt, restrict yourself to the simulation.

Visual reference

Purpose

Show how path difference creates interference fringes, how limiting the wavefront gives diffraction minima, and how a polarizer selects a projection of the electric field.

Representation

A labeled three-panel sketch: left — two slits, rays, path difference dsin⁡θd\sin\theta, and fringes on a screen; middle — one slit with minima asin⁡θ=mλa\sin\theta = m\lambda; right — two polarizers with axes at angle θ\theta and a graph of Malus's law I/I0=cos⁡2θI/I_0 = \cos^2\theta.

Real-world examples

Colors of a soap bubble

Scenario

In a kitchen sink, a soap bubble is lit by white light. The soap film has thickness t=300 nmt = 300\,\text{nm} and refractive index n=1.33n = 1.33. Light reflecting from the outer and inner surfaces of the film interferes. The optical path difference is 2nt=2⋅1.33⋅300 nm=798 nm2nt = 2 \cdot 1.33 \cdot 300\,\text{nm} = 798\,\text{nm}. Because of the π\pi phase shift on reflection at the outer surface, the constructive condition is 2nt=(m+12)λ2nt = (m+\tfrac12)\lambda. For m=1m=1, λ=2nt/1.5=532 nm\lambda = 2nt/1.5 = 532\,\text{nm}, which is green. Thus the bubble appears green in reflected light.

Connection

This scenario uses interference in thin films: the optical path difference Δ=2nt\Delta = 2nt between reflections from the top and bottom surfaces plus a π\pi phase shift on one reflection determines which wavelengths are enhanced. It tests the condition Δ=(m+12)λ\Delta = (m+\tfrac12)\lambda for constructive interference.

Rainbow from a CD

Scenario

A laser pointer with λ=650 nm\lambda = 650\,\text{nm} (red) shines on a CD, which acts as a reflection diffraction grating. The track spacing is d=1.6 μm=1600 nmd = 1.6\,\mu\text{m} = 1600\,\text{nm}. The first-order diffraction angle θ1\theta_1 satisfies sin⁡θ1=λ/d=650/1600=0.406\sin\theta_1 = \lambda/d = 650/1600 = 0.406, so θ1≈24∘\theta_1 \approx 24^\circ. A second-order spot would require sin⁡θ2=2λ/d=1.30>1\sin\theta_2 = 2\lambda/d = 1.30 > 1, so it is not visible. The red spot appears at 24∘24^\circ from the reflected beam.

Connection

This uses diffraction from a periodic grating: the condition dsin⁡θ=mλd\sin\theta = m\lambda for constructive interference of waves from adjacent tracks. It exercises the concept of diffraction orders and the limit ∣sin⁡θ∣≤1|\sin\theta|\le 1.

Phone screen through polarizing sunglasses

Scenario

A phone screen emits unpolarized light of intensity I0=10 W/m2I_0 = 10\,\text{W/m}^2. The screen's built-in polarizer makes the light linearly polarized and halves the intensity: 0.5I0=5 W/m20.5 I_0 = 5\,\text{W/m}^2. Sunglasses with a polarizing filter are at 60∘60^\circ to the screen's polarization. By Malus's law the transmitted intensity is I=5 W/m2⋅cos⁡260∘=1.25 W/m2I = 5\,\text{W/m}^2 \cdot \cos^2 60^\circ = 1.25\,\text{W/m}^2. Rotating the sunglasses to 90∘90^\circ makes the screen nearly black.

Connection

This scenario applies polarization and Malus's law: unpolarized light becomes linearly polarized after passing through a polarizer, and the intensity after an analyzer at angle θ\theta is I=Ipolcos⁡2θI = I_{\text{pol}}\cos^2\theta. It tests the transverse nature of light and the cosine-squared dependence.