Physics · Optics · Chapter notes
Wave Optics · Class 12 Notes
Class 12 Physics notes on Wave Optics: Huygens' principle, coherence and superposition, Young's double slit and fringe width, intensity in interference, single-slit diffraction, polarisation with Malus and Brewster, fringe shift and resolving power, with a JEE Advanced tier and a one-page fact sheet.
In short
Wave optics replaces rays with wavefronts and asks one question: what is the path difference? A path difference of nλ gives a bright fringe and an odd number of half wavelengths gives a dark one, which is all of Young's double slit. Diffraction, polarisation and resolving power follow from the same idea of waves adding up or cancelling.
Contents
- ·How to Read This Set
- 1Huygens' Principle wavefronts, Snell, TIR and Doppler
- 2Superposition and Coherence why two bulbs never interfere
- 3Young's Double Slit path difference and fringe width
- 4Intensity in Interference where the energy actually goes
- 5Diffraction at a Single Slit intensity, and the Fresnel distance
- 6Interference against Diffraction the comparison examiners love
- 7Polarisation Malus, Brewster and the blue sky
- 8Shifting and Changing the Pattern
- 9Resolving Power the limit no lens can beat
- ★Wave Optics · Fact Sheet
How to Read This Set
Sections 1 to 7 are the full syllabus for NEET and JEE Main. Sections 8 and 9 are the JEE Advanced layer, where the pattern is shifted, immersed or lit with white light and you have to work out what happens.
Stop drawing rays. Draw wavefronts, and then compare path lengths.
Every result here comes from one question: by how much does one path exceed the other? Turn that into a phase difference and you have your answer.
- Ray optics assumes light travels in straight lines, which works whenever the obstacle is far larger than the wavelength.
- Visible light has a wavelength around 400 to 700 nm, so a millimetre slit is already thousands of wavelengths wide and rays are fine.
- Shrink the slit towards the wavelength and the light spreads out. No arrangement of straight lines can explain that, so a new model is needed.
- Never start from a formula. Start by asking which two paths you are comparing.
- Convert the path difference into a phase difference with φ = (2π/λ) × Δx.
- Then bright or dark follows immediately, and you will not confuse the interference condition with the diffraction one.
Huygens' Principle
A wavefront is a surface on which every point vibrates in the same phase. A ray is simply the normal to that surface, so rays are a shortcut, not the reality.
| Wavefront | Shape | When you see it |
|---|---|---|
| Spherical | expanding sphere | near a point source |
| Cylindrical | expanding cylinder | from a line source, such as a slit |
| Plane | flat sheet | very far from any source, as with sunlight |
- It gives you the laws of reflection and refraction directly, by drawing the wavelets on the far side of a boundary.
- It predicts that light slows in a denser medium, v = c/μ, which the particle model got exactly backwards.
- It does not explain polarisation, because Huygens assumed the waves were longitudinal. That correction came later.
Snell's law falls straight out of it
- Going from dense to rare the wavefront speeds up, so the refracted ray bends away from the normal.
- At the critical angle the refracted wavefront runs flat along the surface, so r = 90°.
- Past it no wavefront can satisfy the geometry at all, so everything reflects. That is total internal reflection, with sin i(c) = 1/μ.
The Doppler effect for light
For speeds far below c:
Δν/ν = − v(radial)/c and Δλ/λ = + v(radial)/c for a receding source
Motion across the line of sight gives no first-order shift at all.
- A source moving away stretches the wave, so λ increases. That is a red shift, and it is how we know distant galaxies are receding.
- A source moving towards you compresses it, giving a blue shift.
- Worked example: the hydrogen line at 6563 Å arrives 15 Å longer. Then v = cΔλ/λ = 6.9 × 105 m/s, so the source is receding.
- Unlike sound, it makes no difference whether the source or the observer moves. Only their relative radial velocity enters.
Superposition and Coherence
When two waves meet, the displacements simply add. If they arrive in step the result is bigger, and if they arrive exactly out of step they cancel.
- The two sources must be coherent: a constant phase difference that does not drift.
- They must have the same frequency, and nearly the same amplitude for good contrast.
- They must be narrow and close together, or the fringes are too fine to see.
- The light should be monochromatic, otherwise each colour makes its own pattern.
An ordinary source emits light in bursts lasting about 10−9 seconds, each with a random phase. Two independent bulbs therefore change their phase relationship millions of times a second, so the pattern washes out long before your eye can register it. Young's answer was to split one wavefront into two, which is why a double slit works and two lamps do not.
Constructive against destructive
| Constructive | Destructive | |
|---|---|---|
| Phase difference φ | 0, 2π, 4π ... (even multiples of π) | π, 3π, 5π ... (odd multiples) |
| Path difference Δx | nλ | (2n−1)λ/2 |
| Amplitudes | add: a1 + a2 | subtract: a1 − a2 |
| Resulting intensity | (√I1 + √I2)² | (√I1 − √I2)² |
The link between the two rows at the top is worth writing on your hand: φ = (2π/λ) × Δx. Convert once, and every condition in this chapter follows without being memorised separately.
- Young's double slit: one wavefront is divided by two slits, so the two halves keep step forever. This is division of wavefront.
- Thin films, such as a soap bubble or oil on water: one beam is partly reflected and partly transmitted, so the two parts come from the same original wave. This is division of amplitude, and it is why a soap film shows colours.
- A laser: coherent by construction, which is exactly why laser light gives such sharp fringes with no need for a narrow source slit.
Young's Double Slit
Path difference Δx = d sinθ ≈ yd/D
Bright fringe Δx = nλ, so y = nλD/d
Dark fringe Δx = (2n−1)λ/2
Fringe width β = λD/d, the same for every fringe
A worked example
Take λ = 600 nm, d = 1 mm and D = 1 m. Then β = (600 × 10−9 × 1) / 10−3 = 0.6 mm. The fifth bright fringe sits 3.0 mm from the centre, and the angular fringe width is λ/d = 6 × 10−4 radian.
- Wider spacing: increase λ or D, or decrease d.
- Red fringes are wider than blue, since red has the longer wavelength.
- Changing the slit WIDTH does not change β. It only changes the brightness and the contrast. Only the slit separation d matters.
- The central fringe is always bright, because there the two paths are exactly equal.
Drag D and d and see the fringe width respond live, then switch the colour and watch red spread wider than blue.
Intensity in Interference
I = I1 + I2 + 2√(I1I2) cosφ
For equal sources: I = 4I0cos²(φ/2)
Imax/Imin = (√I1 + √I2)² / (√I1 − √I2)²
| If the slit widths are | Amplitudes are | Imax : Imin |
|---|---|---|
| equal | equal | maximum contrast, dark fringes fully black |
| 4 : 1 | 2 : 1 | 9 : 1 |
| 9 : 1 | 3 : 1 | 4 : 1 |
| 16 : 1 | 4 : 1 | 2 : 1 |
- At a bright fringe the intensity is 4I0, not 2I0, because amplitudes add and intensity goes as amplitude squared.
- At a dark fringe it is zero. The energy missing there is exactly the extra energy appearing at the bright fringes.
- Averaged across the screen the intensity is 2I0, precisely what you would get with no interference at all. Energy is redistributed, never lost.
Diffraction at a Single Slit
Now there is only one slit. Light from the top of the slit interferes with light from the bottom, so the wavefront interferes with itself.
Minima a sinθ = nλ, with n = 1, 2, 3 ... never n = 0
Secondary maxima a sinθ = (2n+1)λ/2
Half angular width of the central maximum θ = λ/a
Linear width of the central maximum 2λD/a
With λ = 500 nm, a = 0.1 mm and D = 1 m, the central maximum is 2(500 × 10−9)(1)/10−4 = 10 mm wide, and every other maximum is half that.
- n = 0 is not a minimum. Putting n = 0 into a sinθ = nλ gives the centre of the pattern, which is the brightest point of all.
- The condition for a minimum in diffraction looks exactly like the condition for a maximum in interference. They are opposite. Check which experiment you are in before writing anything.
- Narrower slit means wider pattern. The spreading goes as 1/a, which feels backwards until you accept that light is a wave.
How bright are the secondary maxima?
I = I0 (sin β / β)², with β = πa sinθ / λ
The first secondary maximum is only about 4.7 percent of the central one, and the second about 1.7 percent. That is why the pattern fades so fast.
Where ray optics finally breaks
- A beam through an aperture a spreads by about λ/a, so after a distance z it has widened by roughly zλ/a.
- Set that equal to a itself and you get the Fresnel distance, Z(F) = a²/λ.
- Closer than Z(F) the spreading is negligible and ray optics is safe. Beyond it, diffraction dominates and rays stop meaning anything.
- For a 1 mm aperture at 500 nm, Z(F) is about 2 metres, which is why a laser pointer looks like a straight line across a room but not across a field.
Interference against Diffraction
Polarisation
Interference and diffraction prove light is a wave. Only polarisation proves it is a transverse wave, because a longitudinal wave such as sound cannot be polarised at all.
Malus' law I = I0cos²θ
Brewster's law tan ip = μ, and at that angle the reflected and refracted rays are exactly 90° apart
| Situation | Transmitted intensity |
|---|---|
| unpolarised light through one polariser | always exactly I0/2 |
| then through an analyser at θ | (I0/2) cos²θ |
| analyser at 0° | full intensity |
| analyser at 45° | half |
| analyser at 90° (crossed) | zero, complete extinction |
For glass with μ = 1.5, ip = tan−1(1.5) = 56.3°. For water at μ = 1.33 it is 53.1°. At that angle the reflected light is completely plane polarised, which is exactly how polarising sunglasses cut glare from a wet road or a water surface.
Polarisation by scattering, and why the sky is blue
- Sunlight sets air molecules vibrating, and they re-radiate. But a vibrating charge radiates nothing along its own line of vibration, so light scattered at 90° to the sun comes out plane polarised.
- Scattered intensity goes as 1/λ⁴, which is Rayleigh scattering. Blue at 450 nm scatters about 6 times more than red at 700 nm, so the sky looks blue.
- At sunset the light crosses far more atmosphere, so most of the blue has already been scattered sideways and what reaches you is red.
- Check it yourself: view blue sky 90° from the sun through a polaroid and rotate it. The brightness visibly changes.
Shifting and Changing the Pattern
| Change made | What happens to β | Why |
|---|---|---|
| whole set-up put in water | β becomes β/μ | the wavelength inside is λ/μ |
| D doubled | β doubles | β is proportional to D |
| d doubled | β halves | β is inversely proportional to d |
| slit width increased | no change to β | only brightness and contrast change |
| one slit covered | fringes vanish | a single slit diffraction pattern is left |
| white light used | white centre, coloured edges | each colour has its own β |
A sheet of thickness t and index μ adds an extra path of (μ − 1)t.
The whole pattern shifts by Δy = (μ − 1)t D / d = (μ − 1)t β / λ
It shifts towards the covered slit, and the fringe width β does not change.
- The shift is towards the slit you covered, not away from it, because that path now takes longer and the equal-path point moves across to compensate.
- In white light the centre is white, since every colour has zero path difference there. The first fringe on each side is violet nearest the centre and red furthest, because violet has the shortest wavelength.
- Immersing the apparatus shrinks β by a factor μ, and does not change the number of fringes on the screen in the same way you might guess, so compute rather than assume.
Missing orders in a real double slit
A real double slit has slits of finite width, so you never see pure interference. The fringes sit inside a diffraction envelope set by the slit width.
- Interference maxima need d sinθ = nλ. Envelope zeros need a sinθ = mλ.
- Where those coincide the fringe is missing, and that happens when n / m = d / a.
- So if d = 3a, the 3rd, 6th and 9th orders never appear. If d = 2a, every even order vanishes.
- The number of fringes inside the central envelope is therefore fixed by d/a alone, not by λ or D.
Resolving Power
Diffraction sets a hard limit on how close two objects can be and still be seen as two. No amount of magnification beats it, which is why bigger telescopes are built rather than stronger eyepieces.
Telescope limit of resolution Δθ = 1.22λ/D, so resolving power = D/1.22λ
Microscope limit dmin = 1.22λ/(2μ sinβ)
- A bigger aperture D resolves better, which is the entire reason large telescopes exist.
- A shorter wavelength resolves better. That is why an electron microscope, using electron waves far shorter than light, sees what an optical one never can.
- For a 10 cm telescope at λ = 550 nm, the limit is about 6.7 × 10−6 radian.
- Rayleigh's criterion: two points are just resolved when the central maximum of one falls on the first minimum of the other.
Slide the aperture down and see the Airy discs widen until they overlap. Rayleigh's criterion stops being a sentence.
★ Wave Optics · Fact Sheet
Every rule for revision day. Print this page alone.
WAVEFRONTS
Surface of constant phaseRay is its normal
Spherical, cylindrical, plane.
HUYGENS
Every point is a new sourceEnvelope is the next wavefront
Explains reflection and refraction.
COHERENCE
Constant phase differenceSame frequency, narrow, close
Two bulbs can never do it.
YDSE
Δx = d sinθ ≈ yd/DBright nλ, dark (2n−1)λ/2
β = λD/d.
INTENSITY
I = 4I₀cos²(φ/2)Widths 4:1 gives Imax:Imin 9:1
Average stays 2I₀.
SINGLE SLIT
Minima a sinθ = nλ, n ≠ 0Central width 2λD/a
TWICE every other maximum.
THE SWAP TRAP
nλ is a MAXIMUM in interferencebut a MINIMUM in diffraction.
Check which experiment.
POLARISATION
Proves light is TRANSVERSEOne polariser gives I₀/2
Malus: I = I₀cos²θ.
BREWSTER
tan i(p) = μGlass 1.5 gives 56.3°
Reflected and refracted 90° apart.
IN WATER
λ becomes λ/μso β becomes β/μ
Fringes crowd together.
GLASS SHEET
Extra path (μ−1)tShift = (μ−1)tD/d
TOWARDS the covered slit.
RESOLVING POWER
Telescope 1.22λ/DBigger D or smaller λ is better
Rayleigh: max on first min.
DOPPLER
Δλ/λ = v(radial)/cReceding gives RED shift
Only radial motion counts.
FRESNEL DISTANCE
Z(F) = a²/λ1 mm at 500 nm gives about 2 m
Beyond it, rays are meaningless.
MISSING ORDERS
Vanish when n/m = d/ad = 3a kills orders 3, 6, 9
Set by d/a alone.
BLUE SKY
Rayleigh scattering ∝ 1/λ⁴Blue scatters about 6× red
90° scattered light is polarised.
Before the exam
What the paper actually asks from this chapter
Read next
More physics notes
Now play it.
Reading a chapter and understanding it are different things. In the app this chapter becomes a game you play, a short read, then practice that tests you at every step. A full chapter, understood, in 45 to 60 minutes. Free to start.
- PlayA game built for the concept

- ReadThe short NCERT explainer

- PracticeTimed, until it sticks

Still stuck at 11pm? TarQPro reads the answer you got wrong and teaches the idea behind it, not just the right option.
