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JEE · NEET Physics

Class 12 · Chapter 10

Wave Optics

Overview, notes, short notes, formula sheet, daily practice problems, previous year questions, and videos for this chapter — all in one place.

Wave Optics Formula Sheet

12 formulas across 3 topics in Wave Optics.

1 min read

Updated 2026-07-09 · v1.0.0

Interference & Young's Double Slit Experiment

Two coherent light sources create a stable pattern of bright and dark fringes — the position of each fringe depends only on path difference, measured in a fixed geometric setup.

Δx = d sinθ ≈ dy/D

Path difference in Young's double slit experiment

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Geometry of two slits separated by d, screen at distance D, small-angle approximation for the fringe position y

Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
dseparation between the two slitsm[L]
Ddistance from slits to screenm[L]
ydistance of the point from the central maximum on the screenm[L]

Valid when

  • Requires D ≫ d (small-angle approximation) — standard for all YDSE setups

Δx = nλ (n = 0, ±1, ±2, ...) → bright fringe

Condition for constructive interference (bright fringe)

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
norder of the fringedimensionless (integer)[M⁰L⁰T⁰]

Δx = (2n − 1)λ/2 (n = 1, 2, 3, ...) → dark fringe

Condition for destructive interference (dark fringe)

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Common mistakes

  • Dark fringes occur at HALF-integer multiples of λ, not λ/2 exactly at n=1,2,3... written as (2n−1)λ/2 — easy to mis-index by one term

β = λD/d

Fringe width in YDSE

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Distance between two consecutive bright (or dark) fringes, from the constructive-interference condition applied at consecutive n

Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
βfringe width — spacing between consecutive bright or dark fringesm[L]

Valid when

  • All bright fringes (and all dark fringes) are EQUALLY spaced — β is the same throughout the pattern, not just near the centre

I = I₁ + I₂ + 2√(I₁I₂) cosφ

Resultant intensity from two coherent sources

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Superposition of two waves with amplitudes A₁, A₂ and phase difference φ; I ∝ (resultant amplitude)²

Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
I₁, I₂intensities of the two individual sourcesW/m²[MT⁻³]
φphase difference between the two waves at the pointrad[M⁰L⁰T⁰]

Valid when

  • Requires COHERENT sources (constant phase relationship) — for incoherent sources, intensities simply add with no interference term

I(max) = (√I₁ + √I₂)² , I(min) = (√I₁ − √I₂)²

Maximum and minimum intensity in an interference pattern

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Setting cosφ = +1 and −1 respectively in the resultant intensity formula

Valid when

  • I(min) = 0 only when I₁ = I₂ exactly — otherwise dark fringes are dim but not perfectly dark

Fringe shift = (n − 1)tD/d (equivalently (n−1)t/λ fringes)

Fringe shift when a thin slab is placed in one path of YDSE

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The slab introduces an extra path length (n−1)t in that arm, shifting the entire fringe pattern without changing the fringe width

Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
tthickness of the inserted slabm[L]

Valid when

  • The pattern SHIFTS toward the slab side — fringe width β itself stays unchanged

Common mistakes

  • Inserting a slab shifts the pattern; it does NOT change the fringe width β = λD/d, which depends only on λ, D, d

Diffraction

Diffraction is what happens when the slit itself isn't infinitesimally narrow — different parts of the SAME slit interfere with each other, producing a central bright band flanked by much weaker secondary maxima.

a sinθ = nλ (n = ±1, ±2, ...) → minima

Condition for minima in single-slit diffraction

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
awidth of the single slitm[L]

Valid when

  • Note the reversed role compared to YDSE: this condition gives MINIMA here, while the analogous nλ condition gave MAXIMA in double-slit interference

Common mistakes

  • Do not confuse this with the double-slit bright-fringe condition — in single-slit diffraction, nλ gives dark bands, not bright ones

Width of central maximum = 2λD/a

Width of the central maximum in single-slit diffraction

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Twice the distance to the first minimum on either side of the centre

Valid when

  • The central maximum is TWICE as wide as every other (secondary) maximum — a key qualitative fact about diffraction patterns

θ(min) = 1.22 λ/D (Rayleigh's criterion, circular aperture)

Rayleigh's criterion for resolving power (telescope/eye)

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Two point sources are just resolvable when the central maximum of one falls on the first minimum of the other's diffraction pattern

Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
θ(min)minimum angular separation for two objects to be resolvedrad[M⁰L⁰T⁰]
Ddiameter of the aperture (lens/mirror/pupil)m[L]

Valid when

  • A LARGER aperture gives BETTER resolving power (smaller θ(min)) — the reason large telescopes resolve finer detail

Worth remembering

  • Interference gives EQUALLY bright fringes (energy just redistributed); diffraction gives a bright central band with progressively weaker secondary maxima — a key qualitative distinction between the two phenomena

Polarisation

Polarisation only makes sense for transverse waves — it's direct experimental proof that light is transverse, not longitudinal, since sound waves can never be polarised.

I = I₀ cos²θ

Law of Malus

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
I₀intensity of light after passing through the first (polariser)W/m²[MT⁻³]
θangle between the polariser's and analyser's transmission axesrad[M⁰L⁰T⁰]

Valid when

  • I is maximum (=I₀) when axes are parallel (θ=0°), zero when perpendicular (θ=90°, 'crossed polarisers')

Common mistakes

  • The cos² relates INTENSITY, not amplitude — a common slip is to apply cosθ (not squared) directly to intensity

tanθ(B) = n₂/n₁ , θ(B) + θ(r) = 90°

Brewster's law

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At the polarising (Brewster) angle, the reflected and refracted rays are exactly perpendicular to each other

Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
θ(B)Brewster's (polarising) angle of incidencerad[M⁰L⁰T⁰]
θ(r)angle of refraction at the Brewster anglerad[M⁰L⁰T⁰]

Valid when

  • At exactly this angle, the REFLECTED light is completely (linearly) polarised, perpendicular to the plane of incidence

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