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Class 12 · Physics · Part 2

Chapter 10: Wave Optics

Revision notes, practice numericals, a question bank, assertion and reason questions and answers to the NCERT questions. Tap a group to open it; opening one closes the others.

10.1–10.3Wavefronts and Huygens' principleReflection and refraction explained by waves

Wavefronts

  • A wavefront is a surface of constant phase. Light energy travels along rays, which are perpendicular to the wavefronts.
  • A point source gives spherical wavefronts; a distant source (a star) gives plane wavefronts. A point source at the focus of a convex lens gives a plane wavefront after the lens, and a parallel beam gives a converging spherical wavefront.
Swavefront at twavefront at t + τplane wavefronts
Wavefronts: spherical from a point source, plane from a distant source. Rays are normal to them.

Huygens' principle

  • Every point on a wavefront is a source of secondary wavelets that spread with the speed of the wave. The forward envelope of the wavelets at a later time is the new wavefront.
  • Huygens' construction gives the law of reflection i = r and the law of refraction sin i / sin r = v₁/v₂ = n₂/n₁. On refraction the frequency is unchanged; the speed and wavelength reduce in a denser medium (λ = λ₀/n).
  • A plane wave through a prism or a lens is bent because the light travels more slowly in the thicker glass, tilting or curving the wavefront. Violet travels slower than red in glass.
10.4–10.5Interference and Young's double-slit experimentCoherent sources and fringes

Interference

  • Two waves of the same frequency with a constant phase difference are coherent. Independent sources such as two lamps are incoherent, and give no stable pattern; Young obtained coherent sources by dividing one wavefront with two slits.
  • The resultant intensity is I = I₁ + I₂ + 2√(I₁I₂) cos φ. For equal intensities I = 4I₀ cos²(φ/2): maximum 4I₀, minimum zero. For unequal ones I_max/I_min = (√I₁ + √I₂)² / (√I₁ − √I₂)².
  • Bright fringe: path difference = nλ. Dark fringe: = (n + ½)λ.

Fringes

  • In the double-slit set-up path difference ≈ yd/D. Bright fringes at y_n = nλD/d, dark at (n + ½)λD/d. The fringe width β = λD/d is the same for all fringes, so the pattern is equally spaced. The angular fringe width is λ/d.
  • β increases with λ and D, and decreases when d increases. In water β is reduced by the factor 1/n. With white light the central fringe is white and a few coloured fringes follow.
  • A thin sheet (index n, thickness t) over one slit shifts the pattern by (n − 1)t / λ fringes towards that slit.
S₁S₂PODpath difference S₂P − S₁P ≈ yd/D; fringe width β = λD/d
Young's double-slit set-up.
10.6DiffractionSingle slit

Diffraction at a single slit

  • Light spreads into the geometrical shadow when it passes a slit or edge of size comparable to its wavelength. For a slit of width a: the intensity is zero at sin θ = nλ/a (n = ±1, ±2, …), with a bright central maximum of angular width 2λ/a and weak secondary maxima in between.
  • On a screen at distance D the width of the central maximum is 2λD/a, twice that of the others. A narrower slit gives a wider pattern.
  • Diffraction limits the resolving power of telescopes and microscopes: a larger aperture gives a smaller spread ~ λ/a.
−2λ/a−λ/aλ/a2λ/asingle-slit pattern: minima at sin θ = nλ/a
Single-slit diffraction: the central maximum is twice as wide as the others.
10.7PolarisationTransverse nature of light

Polarised light

  • Light from the Sun or a lamp is unpolarised: the electric vector takes all directions in the transverse plane. A polaroid transmits only the component along its pass axis, giving plane polarised light with half the intensity.
  • Malus' law: I = I₀ cos²θ, where θ is the angle between the polarisation direction and the analyser's axis. Turning the analyser through 360° gives two maxima and two minima; crossed polaroids (θ = 90°) transmit nothing.
  • Only transverse waves can be polarised, so polarisation proves that light is a transverse wave. Interference and diffraction occur for sound as well, polarisation does not.
  • Uses: sunglasses to cut glare, 3D cinema, photography filters, liquid-crystal displays.
unpolarised I₀P₁I₀/2P₂ (θ)I₀/2 · cos²θMalus' law: I = I₀ cos²θ
Two polaroids: Malus' law.
Quick referenceFormulas at a glanceRevise before the exam

Key results

  • Fringe width β = λD/d; bright Δ = nλ, dark Δ = (n + ½)λ
  • Intensity I = 4I₀ cos²(φ/2); φ = 2πΔ/λ
  • Single slit minima a sin θ = nλ; central width 2λD/a
  • Malus I = I₀ cos²θ; unpolarised → polaroid: I₀/2
  • Medium: λ = λ₀/n, v = c/n, frequency unchanged

Common mistakes

  • Using the phase difference in place of the path difference (φ = 2πΔ/λ).
  • Saying the frequency changes on refraction.
  • Forgetting that the intensity through the first polaroid is halved.
  • Using the double-slit β formula for a single slit (its central width is 2λD/a).