Diffraction & Polarization

Waves & Optics · free study notes

Diffraction & Polarization

Subject – Physics (IIT‑JEE / Competitive Exams)
Program – INSPIRE Scholarship

Goal: Build a self‑contained, rigorously‑derived reference that covers the essential theory, key formulae, and subtle points that often appear in competitive exams.


Table of Contents

Section Topics
1 Introduction & Basic Concepts
2 Diffraction – Theory & Applications
3 Polarization – Types & Mathematical Description
4 Tricky Points & Common Pitfalls
5 Hard Practice Question (with solution)

1. Introduction & Basic Concepts

Concept Definition
Wavefront Surface of constant phase.
Coherence Ability of two waves to maintain a fixed phase relationship.
Spatial Coherence Overlap of wavefronts at two points.
Temporal Coherence Overlap of phases at a single point over time.
Diffraction Bending or spreading of waves when encountering an obstacle or aperture.
Polarization Orientation of the electric field vector in an electromagnetic wave.

Key Takeaway: Diffraction requires coherence and finite aperture. Polarization is governed by boundary conditions at interfaces and by the geometry of the source.


2. Diffraction – Theory & Applications

2.1 Huygens–Fresnel Principle

Every point on a wavefront acts as a secondary source emitting spherical wavelets. The resultant field at any point is the superposition of all these secondary waves.

Mathematical form
[ \psi(P)=\frac{e^{ikR}}{i\lambda R}\iint_{S}\psi(Q),e^{ik\Delta},dS ] where (R) is the distance from source to observation point, (\Delta) the extra path length.

2.2 Fraunhofer Diffraction (Far‑Field)

Assumptions: source and observation screen are far compared to aperture size. Resulting integrals turn into Fourier transforms.

2.2.1 Single‑Slit

  • Aperture: width (a), uniform illumination.
  • Condition for minima:
    [ a\sin\theta = m\lambda,\quad m = \pm1,\pm2,\dots ]
  • Intensity distribution:
    [ I(\theta)=I_{0}\left(\frac{\sin\beta}{\beta}\right)^{2},\quad \beta=\frac{\pi a\sin\theta}{\lambda} ]
  • Key formula: sinc‑squared pattern.

2.2.2 Double‑Slit

  • Two slits separated by center‑to‑center distance (d).
  • Total intensity:
    [ I(\theta)=I_{0}\left(\frac{\sin\beta}{\beta}\right)^{2}\cos^{2}\delta,\quad \delta = \frac{\pi d\sin\theta}{\lambda} ]
  • Interference + diffraction: envelope from single‑slit, fringes from inter‑slit separation.

2.2.3 Grating

  • (N) equally spaced slits, spacing (d).
  • Principal maxima condition:
    [ d\sin\theta = m\lambda,\quad m=0,\pm1,\pm2,\dots ]
  • Angular width of maxima:
    [ \Delta\theta \approx \frac{\lambda}{Nd} ]
  • Tunable: can resolve spectral lines.

2.3 Fresnel Diffraction (Near‑Field)

When the observation point is not far, the quadratic term in the path difference cannot be neglected. Fresnel integrals or the Fresnel diffraction integral is used: [ \psi(P)=\frac{e^{ikR}}{i\lambda R}\iint_{S}\psi(Q),e^{ik\frac{(x-X)^{2}+(y-Y)^{2}}{2R}};dx,dy ] Common examples: diffraction by a half‑screen, circular aperture (Airy pattern).

2.4 Diffraction of Light by Circular Apertures (Airy Pattern)

  • Radius (a).
  • Intensity: [ I(\theta)=I_{0}\left(\frac{2J_{1}(\alpha)}{\alpha}\right)^{2},\quad \alpha=\frac{2\pi a\sin\theta}{\lambda} ]
  • First dark ring occurs at (\alpha \approx 3.8317).

2.5 Key Formula Sheet

Scenario Condition Intensity
Single‑slit minima (a\sin\theta=m\lambda) —
Single‑slit maxima (a\sin\theta=(m+1/2)\lambda) —
Double‑slit interference (d\sin\theta=m\lambda) (I=I_{0}\cos^{2}\delta)
Grating maxima (d\sin\theta=m\lambda) (I=I_{0}\frac{\sin^{2}(N\delta)}{\sin^{2}\delta})
Circular (Airy) (\alpha = \frac{2\pi a\sin\theta}{\lambda}) (I=I_{0}\left(\frac{2J_{1}(\alpha)}{\alpha}\right)^{2})

3. Polarization –

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