Shine a laser at two narrow slits and watch light behave as a wave behind them: circular waves spread out from each slit, they add up, and alternating bright and dark fringes appear on the screen. Change the wavelength λ, the slit separation d, the slit width a and the distance to the screen L, cover one slit, switch on white light or send the light one photon at a time — and find out what the fringe spacing Δy = λL/d depends on.
The plane near the slits is the wave field at a magnified scale: bright arcs are wave crests from the two slits, dark “spokes” are directions where the waves cancel. Coloured sheets of light go to the maxima k = 0, 1, 2… on the screen; the yellow line is point P.
Model: each slit is a row of Huygens secondary-wave sources; the screen and the graph are computed with the Fraunhofer formula I = 4I₀·cos²(πd·sinθ/λ)·(sin α/α)². The region near the slits is shown magnified (micrometres), the path to the screen in metres; both scales preserve angles, so the rays from the wave field land exactly on the fringes on the screen. The slits are micrometre-sized so that the waves are visible; for d = 0.1–1 mm the formulas are the same and the fringes are millimetre-sized.
In 1801 Thomas Young passed sunlight through two closely spaced openings and saw on the screen not two spots of light but a whole system of fringes. If light were a stream of tiny particles flying in straight lines, there would be no fringes. The fringes appear because light is a wave: behind the slits the waves bend around the edges (diffraction), overlap and add up (interference). Where a crest of one wave meets a crest of the other, the light is reinforced; where a crest meets a trough, it cancels. Light plus light can give darkness!
d is the slit separation, θ is the angle at which a point of the screen is seen from the slits; Δ is how much longer the path from the farther slit is than from the nearer one
A bright fringe (maximum) is where the path difference equals a whole number of wavelengths; a dark one (minimum) is where it equals a half-integer number; k = 0, ±1, ±2… is the order of the fringe
Δy is the distance between neighbouring bright (or dark) fringes on the screen, L is the distance from the slits to the screen; the formula holds for small angles
a is the slit width; in these directions light from a single slit cancels completely — these are the zeros of the envelope that sets the brightness of the interference fringes
I₀ is the intensity at the centre from one slit; the cos² factor is the interference of two slits (fine fringes), the (sin α/α)² factor is the diffraction by each slit (the envelope)
Young’s experiment is simple: a laser, an opaque plate with two narrow parallel slits, and a screen. By Huygens’ principle each slit itself becomes a source of secondary waves. These waves are born from the same incident wave, so they are coherent — they oscillate in step, with a constant phase difference. In the simulator the horizontal plane near the slits shows the instantaneous wave field: the bright arcs are wave crests running away from the slits, and the dark “spokes” between them are lines where the waves cancel each other all the time.
Where a bright fringe lands is decided by the path difference. To a point P on the screen seen at an angle θ, the wave from the farther slit travels a path longer by Δ = d·sin θ. If this difference holds a whole number of wavelengths, Δ = kλ, the crests arrive together — a maximum of order k. If it is a half-integer, Δ = (k + ½)λ, a crest meets a trough and there is a dark fringe. The lower panel of the simulator makes this visible: drag point P along the graph and watch how the two waves shift relative to each other and what their sum looks like.
For small angles sin θ ≈ tan θ = y/L, and the maxima lie on the screen at equal intervals Δy = λL/d. This gives three main conclusions that are easy to check with the sliders. The longer the wavelength, the wider the fringes: a red laser gives wider fringes than green or blue. The farther the screen, the wider the fringes. And the closer the slits are to each other, the wider the fringes — that is why the slits in Young’s experiment must be very close. By measuring Δy, L and d you can find the wavelength of light: λ = Δy·d/L. This is exactly how Young first measured the wavelength of visible light — about half a micrometre.
Each slit has a finite width a, and light diffracts on it too. So the fringes are not equally bright: they are “covered” by an envelope — the single-slit diffraction pattern with zeros at a·sin θ = mλ (the dashed line on the graph). The narrower the slits, the wider the central hump and the more fringes fit into it. If d/a is an integer, some maxima fall exactly on zeros of the envelope and disappear: for d = 5a the 5th, 10th… orders are missing. Cover one slit — the fine fringes vanish, a broad diffraction band remains, and the brightness at the centre drops not 2 but 4 times: two coherent waves add by amplitude, I ∝ (E + E)² = 4E².
Switch on white light. The central fringe is white — for it Δ = 0 at every wavelength. The side fringes are rainbow-coloured: violet closer to the centre, red farther out, because Δy ∝ λ; further away the coloured fringes of different orders overlap and blur. Finally, the “one photon at a time” mode: even when the light is so weak that only one photon at a time flies through the setup, the dots on the screen gradually build up the same interference fringes. Each photon “passes through both slits” as a wave but hits the screen at a single point — this is wave–particle duality.
First come simulators and problems from this very chapter, then closely related topics of the section.
Optics · Refraction of Light
Optics · Refraction of Light
Optics · Refraction of Light
Optics · Refraction of Light
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Mechanics · Energy