Young's Double-Slit Experiment

For a century after Newton, light was a stream of tiny particles — corpuscles — and the greatest name in physics had said so. Then, around 1803, an English physician-polymath named Thomas Young did something almost embarrassingly simple. He let sunlight through a pinhole to make a single clean beam, split that beam in two (a slip of card edgewise in the beam in his own demonstration; two closely spaced slits in the canonical textbook form), and looked at the wall beyond. Instead of two bright lines, he saw a row of evenly spaced bright and dark bands — fringes — marching across the screen. Particles cannot do that. Two streams of bullets never add up to darkness. But two overlapping waves can: crest on crest builds a bright band, crest on trough cancels to a dark one. The banded pattern was the fingerprint of interference, and it settled the question. Light is a wave. This article is about the experiment that carried that argument and, just as importantly, the geometry that makes it quantitative. Young did not merely show that light interferes; he used the spacing of his fringes to measure the wavelength of light — a length a thousand times smaller than a millimetre — with a ruler and a screen. The whole machine reduces to one line of algebra: the path difference from the two slits to a point on the screen is Δ≈dy/D\Delta \approx dy/D, and the bright fringes fall wherever that equals a whole number of wavelengths. Out of that drops the single formula every exam wants — the fringe spacing β=λD/d\beta = \lambda D/d — and every double-slit numerical you will ever solve. The pattern on the wall is a wavelength, magnified a thousandfold and made visible.

Key takeaways
  • A single monochromatic source lights two narrow slits a distance dd apart; on a screen a distance DD away the two coherent beams overlap and interfere into evenly spaced bright and dark fringes.
  • The path difference from the two slits to a point yy above the centre is Δ≈dy/D\Delta \approx dy/D (small-angle geometry).
  • Bright fringes sit where Δ=nλ\Delta = n\lambda, giving yn=nλD/dy_n = n\lambda D/d; dark fringes where Δ=(n−12)λ\Delta = (n-\tfrac12)\lambda, giving yn=(n−12)λD/dy_n = (n-\tfrac12)\lambda D/d.
  • The fringe spacing (centre-to-centre) is β=λD/d\beta = \lambda D/d — uniform, and the engine of every numerical.
  • Widen the slit separation dd and the fringes crowd together; move the screen back (larger DD) or use a longer λ\lambda and they spread. Immersing the whole apparatus in a medium nn shrinks every fringe: β′=β/n\beta' = \beta/n.
  • Young (1803) used β=λD/d\beta = \lambda D/d backwards to measure the wavelength of light — the first evidence that light is a wave.
  • Key idea: two coherent slits turn an invisible wavelength into a visible ruler — bright fringes at Δ=nλ\Delta = n\lambda, spaced by β=λD/d\beta = \lambda D/d.
The core insight

When one monochromatic source lights two slits dd apart, the path difference to a screen point yy (distance DD away) is Δ≈dy/D\Delta \approx dy/D; bright fringes fall at Δ=nλ\Delta = n\lambda and dark at Δ=(n−12)λ\Delta = (n-\tfrac12)\lambda, so the pattern is a uniform train of fringes spaced by β=λD/d\beta = \lambda D/d — a magnified image of the wavelength itself.

Where this lives today

Young's two-beam interferometer is the ancestor of every precision optical instrument that counts wavelengths. Split one beam into two, recombine them, and the fringes report the path difference between the two arms to a fraction of a wavelength — the working principle of the Michelson interferometer, of the Fabry–Pérot etalons that lock laser frequencies, and, at the grandest scale, of LIGO, whose kilometre-long arms detect gravitational waves by watching interference fringes shift by less than a thousandth of a proton's width. The same fringe geometry calibrates the flatness of optical surfaces, measures the thickness of transparent films, and reads out the tiny displacements in fibre-optic sensors. And the experiment's deepest legacy is conceptual: fire the double slit one photon at a time, or one electron at a time, and the interference pattern still builds up dot by dot — the founding demonstration of quantum superposition, and the experiment Richard Feynman called the one that holds "the only mystery" of quantum mechanics. Young's barcode of light turned out to be a barcode of reality itself.

The physical picture

Start from what the previous article established: two coherent sources — same frequency, a fixed phase relationship — produce a sustained interference pattern, bright where the waves arrive in step and dark where they arrive exactly out of step. Young's genius was in how he made two coherent sources out of ordinary light. Two separate lamps will never do it: each lamp is a crowd of independent atoms whose phases jitter randomly billions of times a second, so their pattern washes out instantly. Young's trick was to take one source and split it. The light passing through slit S1S_1 and the light passing through slit S2S_2 began life at the same wavefront, so whatever random phase wobble the source has, both slits inherit it identically — the phase difference between them stays locked. Two slits, one parent beam: guaranteed coherence. Now follow the two beams to the screen. Consider a point PP a height yy above the central axis. Light from S2S_2 (the farther slit) travels a slightly longer road to reach PP than light from S1S_1. That extra distance is the path difference Δ\Delta. If Δ\Delta happens to be a whole number of wavelengths, the two waves arrive crest-aligned and reinforce — a bright fringe. If Δ\Delta is a half-integer number of wavelengths, they arrive crest-against-trough and cancel — a dark fringe. Straight ahead (y=0y = 0) the two paths are exactly equal, Δ=0\Delta = 0, so the centre of the pattern is always bright: the central maximum. As you move up the screen, Δ\Delta grows steadily, sweeping through λ,2λ,3λ,…\lambda, 2\lambda, 3\lambda, \dots and passing a dark fringe halfway between each — a regular ladder of light and shadow.

Figure
Young's double-slit layout — one source split by two slits d apart, the two paths to a screen point P a height y away on a screen a distance D off, and the extra-path triangle that sets the fringes
One source, two slits — the extra path Δ ≈ d·y/D decides bright or dark source S₁ S₂ d screen P y D (screen distance, ≫ d) fringes bright where Δ = nλ · dark where Δ = (n − ½)λ · spacing β = λD/d

Two length scales make this work, and their ratio is the whole magic. The slit separation dd and the wavelength λ\lambda are microscopic — dd is a fraction of a millimetre, λ\lambda is under a thousandth of that. But the screen distance DD is huge by comparison — a metre or more. The geometry amplifies the tiny wavelength up to the visible fringe spacing by exactly the factor D/dD/d, which in a typical bench setup is around a thousand. That is how a length of 600 nm600\ \mathrm{nm} — utterly invisible — becomes a 0.6 mm0.6\ \mathrm{mm} fringe you can measure with a travelling microscope.

The geometry: path difference to a screen point

Everything rests on one small-angle approximation. Because the screen is far away (D≫dD \gg d), the two rays from S1S_1 and S2S_2 to the point PP are very nearly parallel. Drop a perpendicular from S1S_1 onto the ray from S2S_2: the little right triangle it forms has the slit separation dd as its hypotenuse and the path difference Δ\Delta as the short side opposite the angle θ\theta that the rays make with the axis. So the extra path is

Δ=dsin⁡θ≈dtan⁡θ=d yD(1)\Delta = d\sin\theta \approx d\tan\theta = d\,\frac{y}{D} \qquad (1)

where: dd — the separation between the two slits; yy — the height of PP above the central axis; DD — the slit-to-screen distance; θ\theta — the small angle the rays make with the axis, so small that sin⁡θ≈tan⁡θ=y/D\sin\theta \approx \tan\theta = y/D. The physical reading: the farther up the screen you look (larger yy), the longer the detour the far slit's light must make, and the path difference grows in exact proportion to yy. This linearity is why the fringes come out evenly spaced.

Bright and dark fringes

A bright fringe appears wherever the two waves arrive in step — that is, wherever the path difference is a whole number of wavelengths. Setting Δ=nλ\Delta = n\lambda in equation (1) and solving for the position:

bright: Δ=nλ  ⇒  yn=nλDd,n=0,1,2,…(2)\text{bright: } \Delta = n\lambda \;\Rightarrow\; y_n = \frac{n\lambda D}{d}, \qquad n = 0, 1, 2, \dots \qquad (2)

where: nn is the order of the fringe — n=0n = 0 is the central bright fringe on the axis, n=1n = 1 the first bright fringe on either side, and so on. A dark fringe appears where the waves arrive exactly out of step, which is where the path difference is an odd number of half-wavelengths, Δ=(n−12)λ\Delta = (n - \tfrac12)\lambda:

dark: Δ=(n−12)λ  ⇒  yn=(n−12)λDd,n=1,2,3,…(3)\text{dark: } \Delta = \left(n - \tfrac12\right)\lambda \;\Rightarrow\; y_n = \frac{\left(n - \tfrac12\right)\lambda D}{d}, \qquad n = 1, 2, 3, \dots \qquad (3)

where: the first dark fringe (n=1n = 1) sits at 12\tfrac12 a fringe-spacing above the centre, the second at 1121\tfrac12, and so on — each dark fringe nestles exactly halfway between two bright ones. Notice the bright and dark ladders are interleaved and both are evenly spaced. That regularity is the experiment's signature and the reason a photograph of the fringes looks like a barcode.

Fringe spacing: the master formula

The single most useful quantity is the fringe spacing β\beta — the centre-to-centre distance between two neighbouring bright fringes (equivalently, between two neighbouring dark ones). Subtract the position of the nn-th bright fringe from the (n+1)(n{+}1)-th using equation (2):

β=yn+1−yn=(n+1)λDd−nλDd=λDd(4)\beta = y_{n+1} - y_n = \frac{(n+1)\lambda D}{d} - \frac{n\lambda D}{d} = \frac{\lambda D}{d} \qquad (4)

where: β\beta (fringe spacing, sometimes called the fringe width) is independent of nn — every gap in the pattern is the same size, which is exactly why the fringes are uniform. This one line is the engine of every double-slit numerical: measure β\beta, DD and dd with a ruler and you have solved for λ\lambda; know λ\lambda, DD and dd and you have predicted the whole pattern. Take the standard bench values λ=600 nm\lambda = 600\ \mathrm{nm} (red-orange light), d=1 mmd = 1\ \mathrm{mm} and D=1 mD = 1\ \mathrm{m}:

β=λDd=(600×10−9)(1)1×10−3=6×10−4 m=0.6 mm.\beta = \frac{\lambda D}{d} = \frac{(600\times10^{-9})(1)}{1\times10^{-3}} = 6\times10^{-4}\ \mathrm{m} = 0.6\ \mathrm{mm}.

So the bright fringes sit at y1=0.6 mmy_1 = 0.6\ \mathrm{mm}, y2=1.2 mmy_2 = 1.2\ \mathrm{mm}, y3=1.8 mmy_3 = 1.8\ \mathrm{mm}, and the dark fringes at 0.3 mm0.3\ \mathrm{mm}, 0.9 mm0.9\ \mathrm{mm}, and so on. The wavelength was 600 nm=0.0006 mm600\ \mathrm{nm} = 0.0006\ \mathrm{mm}; the fringe is 0.6 mm0.6\ \mathrm{mm} — a magnification of exactly D/d=1000D/d = 1000. There is also a clean angular version: the angular spacing between fringes is

θfringe=βD=λd=600×10−91×10−3=6×10−4 rad≈0.034∘,(5)\theta_{\text{fringe}} = \frac{\beta}{D} = \frac{\lambda}{d} = \frac{600\times10^{-9}}{1\times10^{-3}} = 6\times10^{-4}\ \mathrm{rad} \approx 0.034^\circ, \qquad (5)

which is handy when the screen distance is not given: the fringes subtend a fixed angle λ/d\lambda/d regardless of how far away you put the screen.

Figure
The intensity across the screen — a uniform train of bright fringes spaced by β equal to λD over d, with the central maximum at the centre and dark fringes exactly halfway between
Intensity along the screen — evenly spaced fringes, spacing β = λD/d = 0.6 mm y (mm) I n=0 123 123 00.61.21.8 0.61.21.8 dark 0.3dark 0.9 β = 0.6 mm every gap is the same width — bright at Δ = nλ, dark exactly halfway between

What changes the pattern

Reading equation (4) as a set of dials tells you how to control the fringes. Longer wavelength λ\lambda (redder light) spreads the fringes; shorter (bluer) crowds them — which is why white light gives a coloured pattern, with each colour's fringes at its own spacing and only the central fringe pure white. Larger screen distance DD spreads them linearly. Larger slit separation dd shrinks them — counter-intuitively, pushing the slits farther apart packs the fringes closer, because dd is in the denominator. And the most-tested variation: immerse the whole apparatus in a transparent liquid of refractive index nn. The frequency is fixed by the source, but the wavelength inside the medium shrinks to λmedium=λ/n\lambda_{\text{medium}} = \lambda/n, so every fringe contracts:

β′=λmediumDd=λDn d=βn(6)\beta' = \frac{\lambda_{\text{medium}} D}{d} = \frac{\lambda D}{n\,d} = \frac{\beta}{n} \qquad (6)

where: β′\beta' is the fringe spacing in the medium and β\beta the value in air. For the 0.6 mm0.6\ \mathrm{mm} pattern dunked in water (n=1.33n = 1.33), β′=0.6/1.33=0.451 mm\beta' = 0.6/1.33 = 0.451\ \mathrm{mm} — the fringes crowd together by a third. This is the same λmedium=λ/n\lambda_{\text{medium}} = \lambda/n rule that governed refraction; here it shows up as a shrinking barcode.

Derivation AFringe spacing β = λD/d from the path-difference geometry

The goal is to obtain the master formula β=λD/d\beta = \lambda D/d from nothing but the geometry of two nearly-parallel rays and the condition for a bright fringe — no calculus, only the small-angle approximation and a subtraction. The strategy is to first pin down the path difference to an arbitrary screen point, then impose "bright means a whole number of wavelengths", and finally take the gap between successive bright fringes.

Step 1. Set up the path difference. Light from the two slits S1S_1 and S2S_2, separated by dd, travels to a point PP a height yy up a screen a distance DD away. Because D≫dD \gg d, the two rays are almost parallel and make almost the same small angle θ\theta with the axis. The far slit's extra path is the short side of a right triangle with hypotenuse dd: Δ=dsin⁡θ\Delta = d\sin\theta.

Step 2. Apply the small-angle approximation. For a distant screen θ\theta is tiny, so sin⁡θ≈tan⁡θ=y/D\sin\theta \approx \tan\theta = y/D. Hence Δ≈d y/D\Delta \approx d\,y/D. This is the linear link between screen position yy and path difference Δ\Delta — the crucial step, and the reason the fringes come out equally spaced.

Step 3. Impose the bright-fringe condition. Constructive interference needs the two waves in step, i.e. a path difference of a whole number of wavelengths: Δ=nλ\Delta = n\lambda. Combine with Step 2: d yn/D=nλd\,y_n/D = n\lambda, so the nn-th bright fringe sits at yn=nλD/dy_n = n\lambda D/d.

Step 4. Take the spacing. The fringe spacing is the distance between consecutive bright fringes: β=yn+1−yn=(n+1)λD/d−nλD/d=λD/d\beta = y_{n+1} - y_n = (n{+}1)\lambda D/d - n\lambda D/d = \lambda D/d. The order nn cancels, so every fringe gap is identical — the pattern is uniform. Numerically, λ=600 nm\lambda = 600\ \mathrm{nm}, d=1 mmd = 1\ \mathrm{mm}, D=1 mD = 1\ \mathrm{m} give β=0.6 mm\beta = 0.6\ \mathrm{mm}, with brights at 0.60.6, 1.21.2, 1.8 mm1.8\ \mathrm{mm} and darks at 0.30.3, 0.9 mm0.9\ \mathrm{mm}. Verified: β = (600e−9 · 1)/(1e−3) = 6e−4 m = 0.6 mm; y₁,y₂,y₃ = 0.6,1.2,1.8 mm; dark 0.3,0.9 mm — recomputed in verify_hs2-youngs-double-slit.py.

Go deeper · Derivation B · 1 minHow the pattern responds to λ, D, d and to immersion in a medium
Derivation BHow the pattern responds to λ, D, d and to immersion in a medium

The goal is to turn β=λD/d\beta = \lambda D/d into a set of predictable responses — what happens to the fringes when you change the colour, move the screen, spread the slits, or sink the whole rig in water — so that a numerical asking "the fringes doubled, what changed?" becomes a one-line proportionality. The strategy is to read each variable off equation (4) as a direct or inverse proportion, then handle immersion through the wavelength-in-a-medium rule.

Step 1. Wavelength and screen distance sit on top, so β∝λ\beta \propto \lambda and β∝D\beta \propto D. Switch from 600 nm600\ \mathrm{nm} to 500 nm500\ \mathrm{nm} light and the fringes shrink in the ratio 500/600500/600; double the screen distance and they double. This is why a second bench with λ=500 nm\lambda = 500\ \mathrm{nm}, d=0.5 mmd = 0.5\ \mathrm{mm}, D=2 mD = 2\ \mathrm{m} gives β=(500×10−9)(2)/(0.5×10−3)=2.0 mm\beta = (500\times10^{-9})(2)/(0.5\times10^{-3}) = 2.0\ \mathrm{mm}.

Step 2. Slit separation sits underneath, so β∝1/d\beta \propto 1/d. Push the slits farther apart and the fringes crowd together — the single most common sign error, because intuition wrongly expects "wider apart" to spread the pattern.

Step 3. Immersion changes the wavelength, not the geometry. Inside a medium of index nn the frequency is unchanged but the wavelength contracts to λmedium=λ/n\lambda_{\text{medium}} = \lambda/n. Substituting into β=λmediumD/d\beta = \lambda_{\text{medium}} D/d gives β′=λD/(nd)=β/n\beta' = \lambda D/(n d) = \beta/n: the whole pattern shrinks by the factor nn.

Step 4. Put in the water number. The β=0.6 mm\beta = 0.6\ \mathrm{mm} air pattern, immersed in water (n=1.33n = 1.33), becomes β′=0.6/1.33=0.451 mm\beta' = 0.6/1.33 = 0.451\ \mathrm{mm}. The fringes crowd inward by about a third — a favourite competitive-exam twist. Verified: second bench β = (500e−9 · 2)/(0.5e−3) = 2.0 mm; immersion β′ = 0.6/1.33 = 0.451 mm — recomputed in verify_hs2-youngs-double-slit.py.

Limiting cases

caseresultmeaning
central point, y=0y = 0Δ=0\Delta = 0, always brightthe two paths are equal — the central maximum is fixed and colour-independent
slit separation d→d \to largeβ=λD/d→\beta = \lambda D/d \to smallfringes crowd together; too large a dd and they blur below resolution
slit separation d→d \to smallβ→\beta \to largefringes spread out; the pattern is easiest to see with closely spaced slits
screen distance D→D \to largeβ→\beta \to largemove the screen back and the fringes spread in proportion
immerse in medium nnβ′=β/n\beta' = \beta/nwavelength shrinks to λ/n\lambda/n, so every fringe contracts by nn
white lightcentral fringe white, sides colouredeach λ\lambda has its own β\beta; only n=0n=0 overlaps for all colours

Worked examples

Board level — the standard fringe pattern (CBSE and ICSE pattern)

In a double-slit experiment the slits are d=1 mmd = 1\ \mathrm{mm} apart and the screen is D=1 mD = 1\ \mathrm{m} away. Monochromatic light of wavelength λ=600 nm\lambda = 600\ \mathrm{nm} is used. Find the fringe spacing and the positions of the first three bright fringes and the first two dark fringes.

Step 1. Fringe spacing from equation (4): β=λD/d=(600×10−9)(1)/(1×10−3)=6×10−4 m=0.6 mm\beta = \lambda D/d = (600\times10^{-9})(1)/(1\times10^{-3}) = 6\times10^{-4}\ \mathrm{m} = \boxed{0.6\ \mathrm{mm}}.

Step 2. Bright fringes at yn=nβy_n = n\beta: y1=0.6 mmy_1 = \boxed{0.6\ \mathrm{mm}}, y2=1.2 mmy_2 = \boxed{1.2\ \mathrm{mm}}, y3=1.8 mmy_3 = \boxed{1.8\ \mathrm{mm}}.

Step 3. Dark fringes at yn=(n−12)βy_n = (n-\tfrac12)\beta: the first at 0.5β=0.3 mm0.5\beta = \boxed{0.3\ \mathrm{mm}} and the second at 1.5β=0.9 mm1.5\beta = \boxed{0.9\ \mathrm{mm}} — exactly halfway between the bright fringes, as they must be.

Step 4. Sense-check: the fringes are equally spaced (0.6 mm0.6\ \mathrm{mm} apart) and the wavelength (0.0006 mm0.0006\ \mathrm{mm}) has been magnified up to a visible 0.6 mm0.6\ \mathrm{mm} by the factor D/d=1000D/d = 1000. If your β\beta had come out in micrometres you divided by DD instead of multiplying.

Board level — a second apparatus and the angular fringe (JEE-Main and NEET pattern)

A double slit with d=0.5 mmd = 0.5\ \mathrm{mm} is lit by green light λ=500 nm\lambda = 500\ \mathrm{nm} and the pattern is caught on a screen D=2 mD = 2\ \mathrm{m} away. Find the fringe spacing. What angle does one fringe subtend at the slits?

Step 1. β=λD/d=(500×10−9)(2)/(0.5×10−3)=2×10−3 m=2.0 mm\beta = \lambda D/d = (500\times10^{-9})(2)/(0.5\times10^{-3}) = 2\times10^{-3}\ \mathrm{m} = \boxed{2.0\ \mathrm{mm}} — more than three times wider than the previous bench, because the light is bluer but the slits are closer and the screen farther.

Step 2. The angular fringe spacing does not need DD: θfringe=λ/d=(500×10−9)/(0.5×10−3)=1×10−3 rad\theta_{\text{fringe}} = \lambda/d = (500\times10^{-9})/(0.5\times10^{-3}) = \boxed{1\times10^{-3}\ \mathrm{rad}}.

Step 3. Cross-check with β\beta: θ=β/D=(2×10−3)/2=1×10−3 rad\theta = \beta/D = (2\times10^{-3})/2 = 1\times10^{-3}\ \mathrm{rad} — the two roads agree.

Competitive level — the whole pattern dunked in water (JEE-Advanced and NEET pattern)

The first apparatus (β=0.6 mm\beta = 0.6\ \mathrm{mm} in air) is submerged in a tank of water, n=1.33n = 1.33, with the source, slits and screen all under water. What is the new fringe spacing?

Step 1. Immersion does not touch DD or dd; it shrinks the wavelength. Inside water λwater=λ/n=600/1.33=451 nm\lambda_{\text{water}} = \lambda/n = 600/1.33 = 451\ \mathrm{nm}, the frequency unchanged.

Step 2. Feed the shrunk wavelength into equation (4), or use the shortcut β′=β/n\beta' = \beta/n directly: β′=0.6/1.33=0.451 mm\beta' = 0.6/1.33 = \boxed{0.451\ \mathrm{mm}}.

Step 3. Physical reading: the fringes crowd inward by a third, because the light "measures out" its bright bands in the shorter in-water wavelength. If a distractor offers 0.6×1.33=0.80 mm0.6\times1.33 = 0.80\ \mathrm{mm} it has multiplied by nn instead of dividing — immersion always shrinks the pattern. Timing note: under 45 seconds once you recognise the immersion shortcut β′=β/n\beta' = \beta/n. Do not re-derive from λwater\lambda_{\text{water}} under exam pressure — spot the "in a medium" cue and divide the air fringe spacing by nn in one step.

Exam traps

dd is the separation, aa is the width. Young's fringe spacing uses the slit separation dd in β=λD/d\beta = \lambda D/d. The slit width aa belongs to single-slit diffraction. Writing β=λD/a\beta = \lambda D/a is the single most common double-slit error — check which length the question gives before you plug.

Dark fringes are at (n−12)λ(n-\tfrac12)\lambda, not nλn\lambda. Bright fringes need a whole number of wavelengths of path difference; dark fringes need a half-integer. Mixing these up shifts every dark position by half a fringe. Memory hook: whole λ\lambda = crest on crest = bright.

Immersion divides β\beta by nn; it does not multiply. Sinking the rig in a medium shrinks the wavelength to λ/n\lambda/n, so β′=β/n\beta' = \beta/n. The fringes get closer, never wider. A slab of glass in one path is a different effect (a fringe shift, not a rescaling) — that is the archetype article, not this one.

Fringe spacing is uniform — do not "average" it. Because β=λD/d\beta = \lambda D/d is independent of the order nn, every gap is identical. A question giving "ten fringes span 6.0 mm6.0\ \mathrm{mm}" means β=6.0/10=0.6 mm\beta = 6.0/10 = 0.6\ \mathrm{mm} straight away; you do not need to find individual positions.

Board scope. Young's double slit is examinable on CBSE, ICSE, JEE, NEET, AP Physics 2, both IB levels, and A-Level 9702 (which writes it as λ=ax/D\lambda = ax/D, with aa their symbol for the slit separation and xx for the fringe spacing — a genuine notation clash with the width-aa convention, so read each board's symbol table). IGCSE 0625 has no wave optics at all — do not revise this for an IGCSE paper. The explicit intensity formula I=4I0cos⁡2(ϕ/2)I = 4I_0\cos^2(\phi/2) is CBSE/JEE/NEET depth; AP, IB and A-Level stay at the path-difference conditions and a qualitative intensity picture.

Origins · 1 minThomas Young and how this was discovered
TY
Thomas Young
1773–1829 · London

Thomas Young was a physician by training and a genuine polymath — he practised medicine in London, helped decipher the Rosetta Stone's Egyptian script, and studied the mechanics of the eye — but physics remembers him for settling the nature of light. In an 1801 Bakerian lecture to the Royal Society he proposed the principle of interference, and soon after demonstrated it with the double-slit arrangement that now carries his name: one source split into two coherent beams that overlap into fringes. Crucially, he did not stop at "light is a wave"; he used the fringe geometry to measure its wavelength, obtaining values close to today's for the visible spectrum — the first measurement of the wavelength of light by interference. His conclusion contradicted Newton's corpuscular authority and was resisted for years, until Fresnel and Arago put the wave theory beyond doubt. The formula β=λD/d\beta = \lambda D/d is his experiment reduced to one line.

History
1690
— Christiaan Huygens publishes Traité de la Lumière, treating light as a wave of secondary wavelets.
1704
— Isaac Newton's Opticks argues light is a stream of corpuscles, and his authority makes the particle view dominant for a century.
1801
— Thomas Young states the principle of interference in his Bakerian lecture to the Royal Society.
1803
— Young demonstrates two-source interference fringes and uses their spacing to measure the wavelength of light.
1818
— Augustin-Jean Fresnel and François Arago put the wave theory on a quantitative footing; the Poisson–Arago bright spot confirms it.

Going further

Texts. NCERT Physics Class 12, Ch. 10 ("Wave Optics"), the section on Young's experiment and fringe width · H. C. Verma, Concepts of Physics Vol. 1, "Light Waves", double-slit interference · Halliday, Resnick and Walker, "Interference", Young's experiment · Cambridge A-Level 9702 topic 15 (two-source interference, λ=ax/D\lambda = ax/D).

Provenance. Standard results. Recompute: β=λD/d=(600×10−9)(1)/(1×10−3)=0.6 mm\beta = \lambda D/d = (600\times10^{-9})(1)/(1\times10^{-3}) = 0.6\ \mathrm{mm}; bright y1,y2,y3=0.6,1.2,1.8 mmy_1, y_2, y_3 = 0.6, 1.2, 1.8\ \mathrm{mm}; dark y1,y2=0.3,0.9 mmy_1, y_2 = 0.3, 0.9\ \mathrm{mm}; angular fringe λ/d=6×10−4 rad=0.034∘\lambda/d = 6\times10^{-4}\ \mathrm{rad} = 0.034^\circ; magnification D/d=1000D/d = 1000; second bench β=(500×10−9)(2)/(0.5×10−3)=2.0 mm\beta = (500\times10^{-9})(2)/(0.5\times10^{-3}) = 2.0\ \mathrm{mm} with θ=λ/d=1×10−3 rad\theta = \lambda/d = 1\times10^{-3}\ \mathrm{rad}; immersion β′=0.6/1.33=0.451 mm\beta' = 0.6/1.33 = 0.451\ \mathrm{mm} (with λwater=600/1.33=451 nm\lambda_{\text{water}} = 600/1.33 = 451\ \mathrm{nm}); "ten fringes span 6.0 mm6.0\ \mathrm{mm}" gives β=0.6 mm\beta = 0.6\ \mathrm{mm}; distractor 0.6×1.33=0.80 mm0.6\times1.33 = 0.80\ \mathrm{mm}.

Prerequisites. Coherence & Interference: Path Difference, Phase & Intensity — where coherent sources, path↔phase, and the bright/dark conditions come from. Leads to. ARCHETYPE: YDSE & Fringe-Width Numericals — the slab-shift, immersion and missing-order problem gym · Single-Slit Diffraction — what the finite slit width aa does to the envelope.

Go deeper (UG). The full field treatment of the double slit — the exact intensity as the coherent sum of two spherical waves, the finite-slit envelope, and the coherence conditions that make the pattern visible — is developed in Young's Double-Slit Experiment in the university optics track. Enrichment only; nothing above depends on it.

How did Young actually measure the wavelength of light with just a screen?

He turned β=λD/d\beta = \lambda D/d around. He could measure the fringe spacing β\beta with a scale, the slit-to-screen distance DD with a ruler, and the slit separation dd under a microscope — all ordinary lengths. Then λ=βd/D\lambda = \beta d / D delivers the wavelength directly. Plugging in the standard numbers, a 0.6 mm0.6\ \mathrm{mm} fringe with d=1 mmd = 1\ \mathrm{mm} and D=1 mD = 1\ \mathrm{m} gives λ=600 nm\lambda = 600\ \mathrm{nm}. It is a beautiful piece of measurement: a length far too small to see is read off from a pattern of visible bands, magnified by the geometric factor D/dD/d. Young's own values for the colours of the spectrum were remarkably close to the modern ones.

Why is the central fringe white when I use white light, but the others are coloured?

At the exact centre (y=0y = 0) the path difference is zero for every wavelength at once, so every colour interferes constructively there — the fringes all pile up and the centre is white. Move off-centre and each colour reaches its first bright fringe at its own spacing, β=λD/d\beta = \lambda D/d: violet (short λ\lambda) closest in, red (long λ\lambda) farthest out. So the first-order fringe smears into a little spectrum, violet edge inward, red edge outward. A few orders out the colours overlap and wash back to near-white. This is why the double slit with white light shows a crisp white centre flanked by rainbow-tinged bands — each colour running its own copy of β=λD/d\beta = \lambda D/d.

What is the difference between the slit separation d and the slit width a?

They are two different lengths that do two different jobs. The separation dd is the gap between the centres of the two slits; it sets the interference fringe spacing β=λD/d\beta = \lambda D/d. The width aa is how wide each slit is on its own; it sets the diffraction envelope through asin⁡θ=mλa\sin\theta = m\lambda (the next article). In a real double slit both act at once — you see closely spaced interference fringes sitting inside a broad diffraction envelope — but for the fringe spacing only dd matters. Watch out for A-Level 9702, which confusingly writes the separation as aa; always check the symbol table before you plug a number in.

Do the fringes really go all the way out forever, or do they fade?

The simple formula β=λD/d\beta = \lambda D/d says the bright fringes march on evenly forever, but in reality they fade for two reasons the formula ignores. First, each slit has a finite width aa, so single-slit diffraction imposes a broad envelope that dims the fringes far from centre and even blanks some out where an interference maximum lands on a diffraction minimum (a "missing order"). Second, the small-angle approximation sin⁡θ≈tan⁡θ\sin\theta \approx \tan\theta used to get Δ=dy/D\Delta = dy/D breaks down at large yy, so the far fringes are not quite evenly spaced. For the central handful of fringes — the ones you actually measure — both effects are negligible and β=λD/d\beta = \lambda D/d is excellent. The finite-width envelope is the subject of single-slit diffraction.

Why does pushing the slits farther apart make the fringes closer, not wider?

Because dd sits in the denominator of β=λD/d\beta = \lambda D/d, so β∝1/d\beta \propto 1/d. Physically, a larger separation dd means the path difference Δ=dy/D\Delta = dy/D grows faster as you move up the screen — you reach the next whole wavelength (the next bright fringe) after a smaller step in yy, so the fringes bunch up. Intuition often expects "slits farther apart" to spread the pattern, which is exactly backwards; it is one of the most reliably tested sign traps in the topic. The reliable move is to trust the formula: dd down below means the fringes shrink when dd grows.

Is Young's experiment on my board, and in what form?

It is on almost every major syllabus: CBSE, ICSE, JEE-Main and Advanced, NEET, AP Physics 2, both IB levels, and A-Level 9702. The one exception is IGCSE 0625, which has no wave optics at all. The depth varies. CBSE, JEE and NEET expect the full treatment including the intensity formula I=4I0cos⁡2(ϕ/2)I = 4I_0\cos^2(\phi/2) and immersion/shift variations. AP, IB and A-Level focus on the path-difference conditions and β=λD/d\beta = \lambda D/d (A-Level writes it λ=ax/D\lambda = ax/D) with a qualitative intensity picture, and generally do not push the cos⁡2\cos^2 formula. Whichever board you sit, the geometry in this article — path difference dy/Ddy/D, bright at nλn\lambda, spacing λD/d\lambda D/d — is the common core.

Before this

Where this leads