CBSE Weightage:

Class 12 — Wave Optics

Class 12 — Wave Optics — chapter strategy, formulas, PYQs, and traps

4 min read

Chapter Overview & Weightage

Wave Optics in Class 12 Physics carries 4–6 marks every year and is one of the most predictable scoring chapters. The questions revolve around Young’s double-slit experiment, single-slit diffraction, and Huygens’ principle.

CBSE Class 12 Board — Wave Optics Weightage

YearMarksQuestion Type
202455-mark long: YDSE derivation + numerical
202343-mark numerical + 1-mark MCQ
202255-mark: single-slit diffraction graph + width
202161+5: polarisation + Huygens construction
202044-mark: fringe-shift due to glass plate

Roughly 6% of the Physics paper. Combined with Ray Optics (also high-weightage), the optics unit alone gives ~10 marks.


Key Concepts You Must Know

Ranked by board frequency:

  • Huygens’ principle — every point on a wavefront is a source of secondary wavelets. Used to derive laws of reflection, refraction.
  • Young’s Double-Slit Experiment (YDSE) — formation of interference, fringe width β=λD/d\beta = \lambda D/d, conditions for max/min.
  • Conditions for sustained interference — coherent sources, equal intensities, monochromatic, narrow slits.
  • Single-slit diffraction — central maximum, minima at asinθ=nλa\sin\theta = n\lambda.
  • Polarisation — Malus’s law I=I0cos2θI = I_0 \cos^2\theta, polarisation by reflection, Brewster’s angle taniB=μ\tan i_B = \mu.
  • Difference between interference and diffraction — comparison table is asked almost every year.

Important Formulas

YDSE fringe width: β=λDd\beta = \dfrac{\lambda D}{d}.

Position of bright fringe: yn=nλDdy_n = \dfrac{n\lambda D}{d}.

Position of dark fringe: yn=(2n1)λD2dy_n = \dfrac{(2n-1)\lambda D}{2d}.

Path difference for max: Δ=nλ\Delta = n\lambda.

Path difference for min: Δ=(n+12)λ\Delta = (n + \tfrac{1}{2})\lambda.

Single-slit minima: asinθ=nλa\sin\theta = n\lambda (n=±1,±2,n = \pm1, \pm2, \ldots).

Width of central diffraction max: W=2λD/aW = 2\lambda D/a (twice the spacing of side fringes).

Brewster’s law: taniB=n\tan i_B = n. At this angle, reflected light is fully polarised.

Malus’s law: I=I0cos2θI = I_0 \cos^2\theta.


Solved Previous Year Questions

PYQ 1 — Fringe width (CBSE 2023, 3 marks)

Q. In a YDSE setup, slits are 1 mm apart, screen 1 m away, light wavelength 600 nm. Find the fringe width.

Solution. β=λD/d=(6×107)(1)/(103)=6×104\beta = \lambda D/d = (6 \times 10^{-7})(1)/(10^{-3}) = 6 \times 10^{-4} m =0.6= 0.6 mm. Always convert wavelength to metres before plugging in.

PYQ 2 — Single-slit width (CBSE 2022, 3 marks)

Q. Light of wavelength 500 nm passes through a slit of width 0.2 mm and falls on a screen 1 m away. Find the width of the central maximum.

Solution.

W=2λDa=2×5×107×12×104=5×103 m=5 mmW = \frac{2\lambda D}{a} = \frac{2 \times 5 \times 10^{-7} \times 1}{2 \times 10^{-4}} = 5 \times 10^{-3} \text{ m} = 5 \text{ mm}

PYQ 3 — Interference vs Diffraction (CBSE 2024, 4 marks)

Q. State three differences between interference and diffraction.

Solution.

InterferenceDiffraction
From two (or more) coherent sourcesFrom a single source via slit/edge
Fringes of equal widthCentral max wider; side fringes diminish
All maxima have ~same intensityCentral max much brighter than side maxima

Difficulty Distribution

  • Easy (40%): Fringe-width plug-in, identifying conditions for interference, Malus’s law numerical.
  • Medium (45%): YDSE derivation, single-slit diffraction graph, Brewster’s angle.
  • Hard (15%): Glass-plate fringe shift, intensity ratio in YDSE, YDSE with mixed wavelengths.

Expert Strategy

Toppers’ approach:

  1. Master the YDSE derivation. Path difference =dsinθdy/D= d\sin\theta \approx d \cdot y/D gives β=λD/d\beta = \lambda D/d in 4 lines. This is a guaranteed 3 marks.

  2. Remember the central-max-is-double rule. Width of central diffraction max = 2λD/a2\lambda D/a. Side maxima are half that wide.

  3. Polarisation = easy 2 marks. Memorise Brewster’s law and Malus’s law. Practise 5 numericals.

  4. Diagrams matter. YDSE setup, single-slit pattern with intensity profile, Huygens’ construction — neat labelled diagrams earn 1 mark each.


Common Traps

Trap 1 — Confusing aa (slit width) with dd (slit separation). YDSE uses dd, single-slit uses aa. Mix them and the answer is off by orders of magnitude.

Trap 2 — Forgetting (2n1)(2n-1) for dark fringes. Bright: yn=nβy_n = n\beta. Dark: yn=(2n1)β/2y_n = (2n-1)\beta/2. Some students confuse the formulas.

Trap 3 — Brewster angle requires tan\tan, not sin\sin. taniB=n\tan i_B = n. Many write siniB=n\sin i_B = n which is total internal reflection — different concept.

Trap 4 — Polariser pairs at 90° give zero, not minimum. I=I0cos290°=0I = I_0\cos^2 90° = 0, exactly zero in the ideal case.