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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.

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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
  1. ·How to Read This Set
  2. 1Huygens' Principle wavefronts, Snell, TIR and Doppler
  3. 2Superposition and Coherence why two bulbs never interfere
  4. 3Young's Double Slit path difference and fringe width
  5. 4Intensity in Interference where the energy actually goes
  6. 5Diffraction at a Single Slit intensity, and the Fresnel distance
  7. 6Interference against Diffraction the comparison examiners love
  8. 7Polarisation Malus, Brewster and the blue sky
  9. 8Shifting and Changing the Pattern
  10. 9Resolving Power the limit no lens can beat
  11. Wave Optics · Fact Sheet
0

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.

The whole chapter in one line

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.

Think it through
Why ray optics had to give up
  • 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.
Trap alert
The habit that fixes this chapter
  • 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.
1

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.

Each point becomes a fresh source. The envelope of the wavelets is the next wavefront.HUYGENS: EVERY POINT ON A WAVEFRONT IS ITSELF A NEW SOURCEpoint sourceSPHERICAL wavefrontclose to the sourcePLANE wavefrontvery far from the sourceTHE CONSTRUCTIONEvery point on a wavefront sends out asecondary wavelet. The envelope of allthose wavelets is the NEXT wavefront.WHAT IT EXPLAINSReflection, refraction and the fact thatlight bends round an edge at all.
Each point becomes a fresh source. The envelope of the wavelets is the next wavefront.
WavefrontShapeWhen you see it
Sphericalexpanding spherenear a point source
Cylindricalexpanding cylinderfrom a line source, such as a slit
Planeflat sheetvery far from any source, as with sunlight
Think it through
What Huygens explains, and what he could not
  • 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

Two media, one shared base AC, two different speeds. The ratio of the sines is forced.SNELL'S LAW, DERIVED FROM WAVEFRONTS ALONEmedium 1, fastmedium 2, slowACBv₁tDv₂tirTHE WHOLE DERIVATIONsin i = v₁t / AC    sin r = v₂t / ACdivide: sin i / sin r = v₁ / v₂ = μ₂ / μ₁WHAT IT SETTLEDLight must travel SLOWER in a densermedium, since μ = c/v. Newton's particlemodel predicted the exact opposite.
Two media, one shared base AC, two different speeds. The ratio of the sines is forced.
Think it through
Refraction at a rarer medium, and total internal reflection
  • 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

Only the radial speed counts

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.

Trap alert
Red shift and blue shift
  • 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.
2

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.

What sustained interference requires
  • 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.
Trap alert
Why two separate bulbs never give fringes

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

ConstructiveDestructive
Phase difference φ0, 2π, 4π ... (even multiples of π)π, 3π, 5π ... (odd multiples)
Path difference Δx(2n−1)λ/2
Amplitudesadd: a1 + a2subtract: a1 − a2
Resulting intensity(√I1 + √I2(√I1 − √I2

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.

Think it through
Two sources that ARE coherent
  • 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.
3

Young's Double Slit

One wavefront, split in two. Everything follows from how much further one path runs.YOUNG'S DOUBLE SLIT: THE PATH DIFFERENCE IS THE WHOLE STORYS1S2dscreenPOyDPATH DIFFERENCEΔx = d sinθ ≈ y d / Dvalid when D is much larger than dBRIGHT when Δx = nλDARK when Δx = (2n−1)λ/2FRINGE WIDTHβ = λD / d
One wavefront, split in two. Everything follows from how much further one path runs.
The four results you need

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.

Think it through
What changes the fringe width, and what does not
  • 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.
Fringes not making sense?
Move the screen and watch the spacing change.

Drag D and d and see the fringe width respond live, then switch the colour and watch red spread wider than blue.

Play this concept in the app
4

Intensity in Interference

Intensity, and where the energy goes

I = I1 + I2 + 2√(I1I2) cosφ
For equal sources:   I = 4I0cos²(φ/2)
Imax/Imin = (√I1 + √I2)² / (√I1 − √I2

If the slit widths areAmplitudes areImax : Imin
equalequalmaximum contrast, dark fringes fully black
4 : 12 : 19 : 1
9 : 13 : 14 : 1
16 : 14 : 12 : 1
Think it through
Interference does not destroy energy
  • 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.
5

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.

Divide the slit into pairs of strips. Each pair cancels when the extra path is half a wavelength.SINGLE SLIT: WHY THE CENTRAL MAXIMUM IS TWICE AS WIDEaplanewavefirst minimumcentral maximumfirst minimumMINIMAa sinθ = nλn = 1, 2, 3 ... never 0CENTRAL MAXIMUMwidth = 2λD / aexactly TWICE the widthof every other maximum
Divide the slit into pairs of strips. Each pair cancels when the extra path is half a wavelength.
Single slit results

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.

Trap alert
Two sign traps in one formula
  • 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?

Intensity across the pattern

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

Think it through
Fresnel distance
  • 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.
6

Interference against Diffraction

Same experiment room, two very different graphs.THE TWO PATTERNS LOOK ALIKE UNTIL YOU MEASURE THEMpositionIINTERFERENCE, two slitsall maxima the SAME brightnessand equally spacedpositionIDIFFRACTION, one slitcentral maximum is WIDE and bright,the rest fade away fastInterference comes from TWO separate wavefronts. Diffraction comes from different partsof the SAME wavefront. That single difference explains every other difference below.
Same experiment room, two very different graphs.
Learn this table as a table. Questions are often lifted straight from a single row.THE COMPARISON THAT ANSWERS MOST ONE-MARK QUESTIONSINTERFERENCEDIFFRACTIONComes fromtwo separate wavefrontsdifferent parts of the SAME wavefrontFringe widthall fringes equally widecentral max is twice the restIntensity of maximaall maxima equally brightfalls off rapidly away from centreMinimaperfectly darknot perfectly darkCondition for maximaΔx = nλa sinθ = (2n+1)λ/2Condition for minimaΔx = (2n−1)λ/2a sinθ = nλNote the conditions are SWAPPED between the two columns. That is the trap.
Learn this table as a table. Questions are often lifted straight from a single row.
7

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.

One polariser halves the intensity. The second one then follows Malus' law.POLARISATION: THE PROOF THAT LIGHT IS A TRANSVERSE WAVEunpolarisedPOLARISERpasses I0/2ANALYSERturned by θθI = I0 cos²θMALUS' LAWθ = 0 gives I0, θ = 90° gives ZEROθ = 45° gives exactly halfBREWSTER'S ANGLEtan i(p) = μglass, μ = 1.5, gives 56.3°reflected and refracted rays are 90° apart
One polariser halves the intensity. The second one then follows Malus' law.
The two laws

Malus' law   I = I0cos²θ
Brewster's law   tan ip = μ, and at that angle the reflected and refracted rays are exactly 90° apart

SituationTransmitted intensity
unpolarised light through one polariseralways 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
Think it through
Brewster's angle, with a number

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

Think it through
Two facts inside one phenomenon
  • 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.
Tier 2
The JEE Advanced layer
Everything so far is complete for NEET and JEE Main. Advanced moves the apparatus: it immerses the whole thing in water, slips a sheet of glass over one slit, or swaps in white light.
8

Shifting and Changing the Pattern

Change madeWhat happens to βWhy
whole set-up put in waterβ becomes β/μthe wavelength inside is λ/μ
D doubledβ doublesβ is proportional to D
d doubledβ halvesβ is inversely proportional to d
slit width increasedno change to βonly brightness and contrast change
one slit coveredfringes vanisha single slit diffraction pattern is left
white light usedwhite centre, coloured edgeseach colour has its own β
A transparent sheet over one slit

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.

Trap alert
Three Advanced results worth carrying
  • 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.

The fine fringes come from the spacing d. The envelope over them comes from the width a.A REAL DOUBLE SLIT: DIFFRACTION DECIDES WHICH FRINGES SURVIVEpositionIdiffraction envelopefrom the slit WIDTH ainterference fringesfrom the slit SPACING dwhere the envelope hits zero, that interference order is MISSINGMaxima need d sinθ = nλ. Envelope zeros need a sinθ = mλ. They coincide when n/m = d/a.So if d/a = 3, orders 3, 6 and 9 never appear, however long you look for them.
The fine fringes come from the spacing d. The envelope over them comes from the width a.
Trap alert
Which orders vanish
  • 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.
9

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.

The two limits

Telescope   limit of resolution Δθ = 1.22λ/D, so resolving power = D/1.22λ
Microscope   limit dmin = 1.22λ/(2μ sinβ)

Think it through
What the formula tells you to do
  • 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.
Want to see the limit for yourself?
Shrink the aperture and watch two stars merge into one.

Slide the aperture down and see the Airy discs widen until they overlap. Rayleigh's criterion stops being a sentence.

Play this concept in the app

★ Wave Optics · Fact Sheet

Every rule for revision day. Print this page alone.

WAVEFRONTS

Surface of constant phase

Ray is its normal
Spherical, cylindrical, plane.

HUYGENS

Every point is a new source

Envelope is the next wavefront
Explains reflection and refraction.

COHERENCE

Constant phase difference

Same frequency, narrow, close
Two bulbs can never do it.

YDSE

Δx = d sinθ ≈ yd/D

Bright 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 ≠ 0

Central width 2λD/a
TWICE every other maximum.

THE SWAP TRAP

nλ is a MAXIMUM in interference

but a MINIMUM in diffraction.
Check which experiment.

POLARISATION

Proves light is TRANSVERSE

One polariser gives I₀/2
Malus: I = I₀cos²θ.

BREWSTER

tan i(p) = μ

Glass 1.5 gives 56.3°
Reflected and refracted 90° apart.

IN WATER

λ becomes λ/μ

so β becomes β/μ
Fringes crowd together.

GLASS SHEET

Extra path (μ−1)t

Shift = (μ−1)tD/d
TOWARDS the covered slit.

RESOLVING POWER

Telescope 1.22λ/D

Bigger D or smaller λ is better
Rayleigh: max on first min.

DOPPLER

Δλ/λ = v(radial)/c

Receding gives RED shift
Only radial motion counts.

FRESNEL DISTANCE

Z(F) = a²/λ

1 mm at 500 nm gives about 2 m
Beyond it, rays are meaningless.

MISSING ORDERS

Vanish when n/m = d/a

d = 3a kills orders 3, 6, 9
Set by d/a alone.

BLUE SKY

Rayleigh scattering ∝ 1/λ⁴

Blue scatters about 6× red
90° scattered light is polarised.

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