Opticsa sinθ = mλ

Single-Slit Diffraction Simulator

Explore Fraunhofer diffraction through a single slit. Adjust slit width and wavelength to see how the diffraction pattern changes.

Parameters
Slit width a
mm
Wavelength λ
nm
Screen distance L
m

Computed
Central max half-width0.000 mm
1st minimum position ±y₁0.000 mm
Formula: y₁ = λL/a
a0.30 mm
λ550 nm
L2.0 m
Δy (central)0.000 mm
±y₁0.000 mm

Single-Slit Diffraction

When light passes through a single narrow slit of width a, it spreads out (diffracts) and produces a characteristic pattern on a screen: a bright central maximum flanked by weaker secondary maxima separated by dark minima. This is Fraunhofer (far-field) diffraction.

Diffraction occurs because each point across the slit acts as a secondary source (Huygens' principle). The waves from all these sources interfere at the screen — constructively near the centre, destructively at the minima.

Dark Fringes (Minima)

The minima occur where the contributions from the top and bottom halves of the slit exactly cancel. The condition is a sinθ = mλ for integers m ≠ 0. For small angles, the position of the m-th minimum on the screen is y_m = mλL/a.

Central Maximum Width

The central bright maximum spans from the first minimum on one side to the first minimum on the other. Its half-width is θ ≈ λ/a. A narrower slit (smaller a) diffracts more, spreading the central peak wider. A wider slit gives a narrower, more intense central peak.

💡Set the slit width to 0.1 mm (very narrow) and notice the very broad central maximum. Increase to 1.0 mm and the pattern sharpens dramatically. This inverse relationship is fundamental to Fourier optics.

Intensity Formula

The intensity at position y on the screen follows the sinc-squared function: I = I₀(sinα/α)² where α = πay/(λL). The secondary maxima have intensities roughly 4.7%, 1.6%, and 0.8% of the central maximum.

Order mPosition y_mIntensity (relative)
0 (central max)0100%
1 (1st minimum)λL/a0%
1.5 (1st secondary max)≈1.43λL/a≈4.7%
2 (2nd minimum)2λL/a0%
2.5 (2nd secondary max)≈2.46λL/a≈1.6%

Single-Slit Diffraction Formulas

Intensity Distribution (Fraunhofer)

Minima Condition

Minimum Position on Screen

Central Maximum Half-Width

SymbolNameUnit
aSlit widthm (or mm)
λWavelengthm (or nm)
LScreen distancem
mDiffraction order (nonzero integer)
αPhase parameter πa sinθ/λrad
I₀Central intensityW/m²

Frequently Asked Questions

Why does a narrower slit produce a wider diffraction pattern?

This is a consequence of the uncertainty principle and Fourier theory. The slit constrains the transverse position of photons (Δx = a). A smaller Δx requires a larger spread in transverse momentum (Δp_y), corresponding to a wider angular spread. Mathematically, the pattern width scales as λ/a.

What is the difference between single-slit diffraction and double-slit interference?

Double-slit interference produces equally-spaced fringes of roughly equal brightness (cos² pattern). Single-slit diffraction produces a broad central peak with weaker, unequally-spaced secondary maxima (sinc² pattern). In practice, double-slit patterns are modulated by the single-slit envelope of each slit.

Why is there no minimum at m = 0?

At m = 0 (the centre), all path differences are zero — every wavelet from the slit arrives in phase. The waves add completely constructively, giving the bright central maximum. Minima only occur for m ≠ 0 where path differences produce cancellation.

How does wavelength affect the pattern?

Longer wavelengths diffract more, so the pattern spreads further: Δy = λL/a. Red light (700 nm) produces a wider central maximum than blue light (450 nm) with the same slit. White light produces coloured fringes outside the white central peak.

What is Fraunhofer diffraction?

Fraunhofer (far-field) diffraction applies when the screen is far enough from the slit that the wavefronts arriving at any screen point are essentially plane waves. The condition is L ≫ a²/λ. For visible light and mm-scale slits this is typically satisfied at distances > 1 m.