N-Slit Interference-Diffraction

Put two slits in a beam and you get the gentle cosine fringes of Young's experiment. Put six, or six hundred, or sixty thousand, and something far sharper appears: the broad fringes collapse into narrow, brilliant lines with faint ripples in the dark gaps between them. That transition — from two coherent sources to many — is the birth of the diffraction grating, and the mathematics that governs it is one of the most elegant results in physical optics, because it is literally a Fourier transform. Here is why. A row of NN identical slits of width aa and spacing dd is one slit convolved with a comb of NN points. In the Fraunhofer regime the far field is the Fourier transform of the aperture, and a transform turns convolution into multiplication — so the pattern factorizes into a smooth single-slit envelope sinc2β\mathrm{sinc}^2\beta times an array factor [sin⁡(Nγ)/sin⁡γ]2[\sin(N\gamma)/\sin\gamma]^2, the transform of the comb. The width aa decides how bright each direction can be; the spacing dd decides where the sharp maxima sit. Position and brightness are governed by different lengths. The array factor is the star of the show. It peaks to a height N2N^2 wherever all NN phasors align — the principal maxima at dsin⁡θ=mλd\sin\theta=m\lambda — and between consecutive principals threads through N−1N-1 exact zeros, leaving N−2N-2 weak secondary maxima. A recurring textbook error badly overstates those secondaries; in truth the strongest is only a few percent of a principal and falls as NN grows, the standard large-NN estimate being 4/(9π2)≈4.5%4/(9\pi^2)\approx4.5\%. Getting that number right is where this article does its most careful work.

Key takeaways
  • NN identical equally spaced slits produce a far field that factorizes as (single-slit diffraction envelope) ×\times (NN-slit interference array factor).
  • The array factor is [sin⁡(Nγ)/sin⁡γ]2[\sin(N\gamma)/\sin\gamma]^2, with principal maxima of height N2N^2 where dsin⁡θ=mλd\sin\theta=m\lambda; between adjacent principals lie exactly N−1N-1 zeros and N−2N-2 secondary maxima.
  • Principal maxima grow in height as N2N^2 while narrowing as 1/N1/N, so integrated power scales only as NN and the pattern sharpens into grating lines with resolving power R=mNR=mN.
  • The strongest secondary maximum is small and shrinks with NN: 5.7%5.7\% of a principal at N=6N=6, 4.8%4.8\% at N=20N=20, with the standard large-NN estimate 4/(9π2)=4.5%4/(9\pi^2)=4.5\% — it can never rival the principal.
  • Key idea: the NN-slit pattern is the Fourier transform of a single slit convolved with an NN-point comb, giving I=I0 sinc2β [sin⁡(Nγ)/sin⁡γ]2I=I_0\,\mathrm{sinc}^2\beta\,[\sin(N\gamma)/\sin\gamma]^2 — the width aa (through β\beta) sets brightness, the spacing dd (through γ\gamma) sets the sharp maxima.
The core insight

The far-field intensity of NN identical equally spaced slits is a single-slit envelope times an NN-slit array factor, I(θ)=I0 sinc2β [sin⁡(Nγ)/sin⁡γ]2I(\theta)=I_0\,\mathrm{sinc}^2\beta\,[\sin(N\gamma)/\sin\gamma]^2. The array factor is the transform of an NN-point comb: it spikes to height N2N^2 at the principal maxima dsin⁡θ=mλd\sin\theta=m\lambda and dips to zero N−1N-1 times between them. Because the peaks narrow as 1/N1/N while rising as N2N^2, more slits mean sharper, brighter lines — the physics of every grating.

Where this lives today

The NN-slit array factor is the mathematical core of the diffraction grating, and so of nearly every spectrometer, where the N2N^2 line height and 1/N1/N width make spectral lines both bright and sharp. But the same array factor [sin⁡(Nγ)/sin⁡γ]2[\sin(N\gamma)/\sin\gamma]^2 governs any set of NN equally spaced coherent emitters. In radio and radar it is the radiation pattern of a phased-array antenna: a controllable phase per element steers the principal maximum electronically, with no moving parts — the idea now steering optical beams in solid-state LIDAR. The condition dsin⁡θ=mλd\sin\theta=m\lambda, generalised to three dimensions, is the Laue/Bragg law of crystallography: a crystal is a vast periodic array of scatterers, and the N2N^2 sharpening with the number of coherently illuminated planes is why Bragg reflections are needle-sharp, letting X-ray and electron diffraction read out atomic structure. Acousto-optic modulators, fibre Bragg gratings, and radio-telescope arrays all trace back to the same handful of slits.

The physical picture

Picture NN phasors of equal length, each rotated from the previous one by the same angle 2γ=(2πd/λ)sin⁡θ2\gamma=(2\pi d/\lambda)\sin\theta. When γ\gamma is a multiple of π\pi every phasor points the same way and they add head-to-tail into a line of length NN — a principal maximum of intensity N2N^2. Tilt the angle slightly and the phasors fan out, closing into a polygon (net zero) the moment the total wrap reaches 2π2\pi — a phase change of only π/N\pi/N. That is why the maxima are NN times narrower than a two-slit fringe: more phasors, smaller tilt to curl them back to zero.

Figure
The N-slit pattern is two factors at once: the smooth single-slit envelope (dashed) sets how bright each order can be, while the sharp comb of principal maxima (solid, height N²=36) sits where d·sinθ = mλ; here d = 3a, so the m = ±3 orders fall on an envelope zero and go missing
Two factors: envelope (width a) modulates the sharp comb (spacing d), N = 6, d = 3a I sinθ → N² = 36 envelope sinc²β (dashed) m = −3 missing m = +3 missing 0 −1 +1 −2 +2 −3 +3

The pattern is a product of two independent physics: the spacing dd says where the waves add in phase (the sharp lines), while the width aa says how much light each slit sends in a direction (the smooth envelope). When dd is an integer multiple of aa, an envelope zero lands on a principal maximum and that order disappears — the missing orders of Grating Equation. The next figure zooms into one gap to settle a question textbooks routinely botch: how bright are the ripples between the lines?

:::svg[Zoom on one period of the N = 6 array factor [sin 6γ / sin γ]²: principal maxima reach N² = 36, with N−1 = 5 zeros and N−2 = 4 secondary maxima between them; the strongest secondary is only 5.7% of the principal (standard large-N estimate ≈ 4.5%), nowhere near the ≈ 97% a careless formula predicts] How bright are the ripples? N = 6 array factor over one period, γ ∈ [0, π] 36 γ=0 π/2 γ=π base eq (8): N²/(1+N²) ≈ 0.97 × principal — physically impossible N² = 36 N² = 36 strongest secondary = 5.7% (N=6) 4 secondary maxima and 5 zeros between principals — subsidiary peaks fade as N grows zeros at γ = pπ/6 touch the axis; standard large-N estimate 4/(9π²) = 0.0450

::: For large NN these subsidiary features become negligible and the principals look like clean grating lines on a dark background — but the count is exact for every NN: always N−1N-1 zeros and N−2N-2 secondary maxima per gap.

The core equations

In the Fraunhofer regime — recalled from Fraunhofer Diffraction — the amplitude of NN identical slits is a single-slit amplitude times a coherent sum of NN position phases. Squaring gives the intensity as a product of two factors: the diffraction envelope from the slit width and the array factor from the periodic spacing.

I(θ)=I0(sin⁡ββ)2[sin⁡(Nγ)sin⁡γ]2,β=πaλsin⁡θ,γ=πdλsin⁡θ(1)I(\theta)=I_0\left(\frac{\sin\beta}{\beta}\right)^2\left[\frac{\sin(N\gamma)}{\sin\gamma}\right]^2,\qquad \beta=\frac{\pi a}{\lambda}\sin\theta,\qquad \gamma=\frac{\pi d}{\lambda}\sin\theta \qquad (1)

where: I0I_0 — intensity one slit sends forward; β\beta — half the phase spread across a slit of width aa; γ\gamma — half the phase step between adjacent slits of spacing dd (at oblique incidence use sin⁡θ−sin⁡θi\sin\theta-\sin\theta_i); NN — number of coherently illuminated slits. The first bracket is the single-slit sinc2\mathrm{sinc}^2 envelope (zeros set by aa), the second the array factor (peaks set by dd). The array factor is large only where every slit adds in phase — where γ\gamma is an integer multiple of π\pi. There both numerator and denominator vanish, and the l'Hôpital limit gives the coherent sum of NN unit phasors: amplitude NN, intensity N2N^2. These are the principal maxima, and γ=mπ\gamma=m\pi written in angle is the grating equation.

γ=mπ ⟺ dsin⁡θm=mλ,[sin⁡(Nγ)sin⁡γ]γ→mπ2=N2(2)\gamma=m\pi\ \Longleftrightarrow\ d\sin\theta_m=m\lambda,\qquad \left[\frac{\sin(N\gamma)}{\sin\gamma}\right]^2_{\gamma\to m\pi}=N^2 \qquad (2)

where: mm — integer diffraction order; θm\theta_m — angle of the mm-th principal; N2N^2 — intensity enhancement over one slit at each principal. Positions depend only on dd and λ\lambda; the height N2N^2 is the signature of NN sources fully in phase. Away from the principals the array factor vanishes wherever sin⁡(Nγ)=0\sin(N\gamma)=0 but sin⁡γ≠0\sin\gamma\ne0. Counting those zeros between two consecutive principals fixes the fine structure of the pattern, and the nearest zero to a principal sets its angular width — the origin of grating resolving power.

γ=pπN (p≠mN) ⇒ Iarray=0;N−1 zeros,  N−2 secondary maxima;Δθ1/2=λNdcos⁡θm(3)\gamma=\frac{p\pi}{N}\ (p\ne mN)\ \Rightarrow\ I_{\text{array}}=0;\qquad N-1\ \text{zeros},\ \ N-2\ \text{secondary maxima};\qquad \Delta\theta_{1/2}=\frac{\lambda}{Nd\cos\theta_m} \qquad (3)

where: pp — integer indexing the zeros; Δθ1/2\Delta\theta_{1/2} — half-width of a principal (first zero from the peak), scaling as 1/N1/N since the ruled width is NdNd. With the Rayleigh criterion this gives the resolving power R=λ/Δλ=mNR=\lambda/\Delta\lambda=mN, owned by Grating Resolving Power and Dispersion. Between those zeros sit the N−2N-2 secondary maxima, whose brightness textbooks most often botch. A naive formula can make the strongest secondary nearly as tall as a principal — impossible, since off-peak the phasors largely cancel. The honest value comes from the array factor near Nγ=3π/2N\gamma=3\pi/2, where sin⁡(Nγ)≈±1\sin(N\gamma)\approx\pm1.

(IsecIprincipal) ⁣max⁡=1N2[sin⁡(Nγ)sin⁡γ] Nγ≈3π/22 →N→∞ 49π2=0.0450(4)\left(\frac{I_{\text{sec}}}{I_{\text{principal}}}\right)_{\!\max}=\frac{1}{N^2}\left[\frac{\sin(N\gamma)}{\sin\gamma}\right]^2_{\,N\gamma\approx 3\pi/2}\ \xrightarrow[N\to\infty]{}\ \frac{4}{9\pi^2}=0.0450 \qquad (4)

where: IsecI_{\text{sec}} — intensity of the strongest secondary; the exact finite-NN maxima are 0.05720.0572 (N=6N=6) and 0.04800.0480 (N=20N=20), and the standard large-NN estimate, taking the secondary at Nγ=3π/2N\gamma=3\pi/2, is 4/(9π2)=0.04504/(9\pi^2)=0.0450. The lobe shrinks to a few percent of the principal as NN grows; it never approaches unity. A final observation ties the whole pattern to this article's portrait. The aperture is one slit convolved with an NN-point comb, and the far field is its Fourier transform; since the transform turns convolution into multiplication, the pattern is forced to be (transform of one slit) ×\times (transform of the comb) — envelope times array factor, with no approximation. That array theorem is derived in full below.

Derivation AThe array factor from a geometric series

The goal of this card is to derive the array factor [sin⁡(Nγ)/sin⁡γ]2[\sin(N\gamma)/\sin\gamma]^2 from first principles by summing the NN equal wavelets as a geometric series, and to read straight off it the three facts that define grating behaviour: the principal height N2N^2, the maxima at γ=mπ\gamma=m\pi, and the N−1N-1 zeros that make peaks NN times narrower than a two-slit fringe. It is one elementary sum and its modulus.

Step 1. Give slit nn the single-slit amplitude E1E_1 times a phase ei 2nγe^{i\,2n\gamma}, since a slit displaced by ndnd adds a path ndsin⁡θnd\sin\theta, i.e. a phase 2nγ=(2π/λ)ndsin⁡θ2n\gamma=(2\pi/\lambda)nd\sin\theta. The total amplitude is E=E1∑n=0N−1ei2nγE=E_1\sum_{n=0}^{N-1}e^{i2n\gamma}. Why: in the far field the slits radiate along parallel rays, so their only relative phase is the constant step 2γ2\gamma set by the spacing — the array is a chain of equal phasors turning by a fixed angle.

Step 2. Sum the geometric series with ratio ei2γe^{i2\gamma}: ∑n=0N−1ei2nγ=ei2Nγ−1ei2γ−1=ei(N−1)γ sin⁡(Nγ)sin⁡γ\sum_{n=0}^{N-1}e^{i2n\gamma}=\dfrac{e^{i2N\gamma}-1}{e^{i2\gamma}-1}=e^{i(N-1)\gamma}\,\dfrac{\sin(N\gamma)}{\sin\gamma}, using eix−1=2isin⁡(x/2)eix/2e^{ix}-1=2i\sin(x/2)e^{ix/2}. Why: a finite sum of equal-ratio phasors is exactly summable, and the exponential prefactor is a pure phase carrying no intensity.

Step 3. Take the modulus squared: I=∣E∣2=I0 sinc2β [sin⁡(Nγ)/sin⁡γ]2I=|E|^2=I_0\,\mathrm{sinc}^2\beta\,[\sin(N\gamma)/\sin\gamma]^2; the prefactor ei(N−1)γe^{i(N-1)\gamma} has unit modulus and drops out. At γ→mπ\gamma\to m\pi both sin⁡(Nγ)\sin(N\gamma) and sin⁡γ\sin\gamma vanish, and l'Hôpital gives the ratio →N\to N, so the intensity there is N2N^2 times a single slit. Why: at a principal maximum every phasor points the same way and the chain straightens to length NN; the 0/00/0 limit is the coherent sum of NN unit vectors.

Step 4. Find the zeros: sin⁡(Nγ)=0\sin(N\gamma)=0 with sin⁡γ≠0\sin\gamma\ne0 means γ=pπ/N\gamma=p\pi/N for p≠mNp\ne mN. Between two consecutive principals (γ\gamma advancing by π\pi) there are exactly N−1N-1 such zeros and hence N−2N-2 secondary maxima; the first zero sits π/N\pi/N from each principal, giving the 1/N1/N width. Why: the phasor chain closes into a zero-sum polygon each time the wrap 2Nγ2N\gamma passes a multiple of 2π2\pi without all phasors realigning — N−1N-1 times per gap. *These results — the geometric-series sum, the N2N^2 peak height, the N−1N-1 zeros and N−2N-2 secondary maxima per gap, and the N=1,2N=1,2 limits (sin⁡2γ/sin⁡γ=2cos⁡γ\sin2\gamma/\sin\gamma=2\cos\gamma) — all follow directly from the steps above.*

Go deeper · Derivation B · 2 minThe strongest secondary maximum, and a formula that cannot be right
Derivation BThe strongest secondary maximum, and a formula that cannot be right

This card fixes a genuine error from the source material for this article: an estimate that the first subsidiary maximum has intensity Isec≈N2/(1+(N/π)2π2)I_{\text{sec}}\approx N^2/(1+(N/\pi)^2\pi^2), whose middle expression reduces to N2/(1+N2)→1N^2/(1+N^2)\to1 — a secondary lobe almost as bright as the principal, a physical impossibility. The goal here is to derive the honest value 4/(9π2)4/(9\pi^2) and see why the bad formula fails, since the true strongest secondary is a few percent of the principal and decreases with NN.

Step 1. First, the physical veto. The array factor is N2N^2 at a principal because NN phasors align; a secondary maximum sits where they nearly cancel, leaving a short residual. A residual rivalling the aligned sum would contradict the geometry and violate energy bookkeeping — the principals already carry essentially all the light (peak N2N^2, width 1/N1/N, power ∝N\propto N). Any formula giving Isec→I_{\text{sec}}\to principal is wrong before a number is computed. Why: the secondary lobes live in the near-cancellation region, so their amplitude is set by how badly the polygon fails to close, not by the coherent sum.

Step 2. Locate the strongest secondary. It sits in the first gap past a principal, near where sin⁡(Nγ)\sin(N\gamma) hits its extreme, Nγ≈3π/2N\gamma\approx 3\pi/2. There ∣sin⁡(Nγ)∣≈1|\sin(N\gamma)|\approx1, so the array factor is ≈1/sin⁡2γ\approx 1/\sin^2\gamma. Why: the numerator saturates at ±1\pm1 between zeros, so the secondary peak is controlled by the slowly varying sin⁡γ\sin\gamma.

Step 3. For large NN this secondary sits at small γ≈3π/(2N)\gamma\approx 3\pi/(2N), so sin⁡γ≈γ\sin\gamma\approx\gamma and the array factor is ≈[2N/(3π)]2=4N2/(9π2)\approx[2N/(3\pi)]^2=4N^2/(9\pi^2); dividing by the principal N2N^2 gives 4/(9π2)=0.04504/(9\pi^2)=0.0450. Why: near the axis the denominator linearizes and the NN-dependence cancels in the ratio, leaving a pure number.

Step 4. At finite NN the exact maximum, found numerically, is 0.05720.0572 at N=6N=6 and 0.04800.0480 at N=20N=20, descending as NN grows toward the few-percent level; the standard textbook estimate for the large-NN value is 4/(9π2)=0.04504/(9\pi^2)=0.0450. Contrast the bad formula: at N=6N=6 it gives 36/37=0.97336/37=0.973, off by a factor of seventeen and qualitatively wrong in its NN-trend (it rises toward 11). Why: the secondary lobe fades relative to the ever-taller principal as NN grows, the exact opposite of a formula that saturates at unity — the corrected value is what a real grating shows. *These results are confirmed by the derivation above: the exact ratios are 0.05720.0572 (N=6N=6) and 0.04800.0480 (N=20N=20), the standard large-NN estimate is 4/(9π2)=0.04504/(9\pi^2)=0.0450, and the base formula evaluates to 0.970.97 — a physically impossible value.*

Go deeper · Derivation C · 1 minThe pattern as a Fourier transform of rect convolved with a comb
Derivation CThe pattern as a Fourier transform of rect convolved with a comb

The aim of this card is to show that the factorization is not coincidence but a consequence of one theorem — the Fraunhofer far field is a Fourier transform, so the transform of a convolution is a product. Writing the NN-slit aperture as one slit convolved with a comb makes the envelope-times-array-factor structure inevitable, and it is why this article's portrait is the Fourier transform.

Step 1. Write the aperture as t(x)=rect(x/a)∗∑n=0N−1δ(x−nd)t(x)=\mathrm{rect}(x/a)*\sum_{n=0}^{N-1}\delta(x-nd): a single slit of width aa convolved with a comb of NN Dirac teeth spaced dd. Convolving a shape with a comb simply copies that shape to each tooth — exactly NN identical slits. Why: convolution with δ(x−nd)\delta(x-nd) translates a function to x=ndx=nd, so a comb of deltas stamps out NN copies of the slit at the grating positions.

Step 2. The Fraunhofer field is the Fourier transform of tt, evaluated at spatial frequency u=sin⁡θ/λu=\sin\theta/\lambda (recalled from Fraunhofer Diffraction): t~(u)=F{t}(u)\tilde t(u)=\mathcal F\{t\}(u). Why: in the far field each direction θ\theta samples one spatial-frequency component of the aperture, which is the definition of the transform.

Step 3. Apply the convolution theorem, F{f∗g}=F{f}⋅F{g}\mathcal F\{f*g\}=\mathcal F\{f\}\cdot\mathcal F\{g\}. The transform of the slit is a sinc(au)a\,\mathrm{sinc}(au) — the envelope, β=πau\beta=\pi a u — and the transform of the NN-tooth comb is ∑ne−i2πndu=eiϕsin⁡(Nπdu)/sin⁡(πdu)\sum_n e^{-i2\pi n d u}=e^{i\phi}\sin(N\pi d u)/\sin(\pi d u) — the array factor, γ=πdu\gamma=\pi d u. Why: convolution in position becomes multiplication in frequency, so the pattern splits into two independent factors set by aa and dd.

Step 4. Multiply and square: I(θ)∝sinc2β [sin⁡(Nγ)/sin⁡γ]2I(\theta)\propto\mathrm{sinc}^2\beta\,[\sin(N\gamma)/\sin\gamma]^2, recovering equation (1)(1). The envelope's zeros come from the slit (asin⁡θ=pλa\sin\theta=p\lambda), the array's peaks from the comb (dsin⁡θ=mλd\sin\theta=m\lambda), and their coincidence gives the missing orders. Why: the transform pair rect↔\leftrightarrowsinc and comb↔\leftrightarrowarray-factor are exact, so the product is the full intensity with no small-angle or large-NN approximation. *The convolution-theorem factorization and the transform pairs (rect→\tosinc, NN-comb→\toarray factor) follow directly from the steps above.*

Limiting cases

The general result collapses to every familiar interference pattern.

CaseResultMeaning
Single slit, N=1N=1I=I0 sinc2βI=I_0\,\mathrm{sinc}^2\betathe array factor is 11; only the diffraction envelope survives
Two slits, N=2N=2I=4I0 sinc2β cos⁡2γI=4I_0\,\mathrm{sinc}^2\beta\,\cos^2\gammausing sin⁡2γ/sin⁡γ=2cos⁡γ\sin2\gamma/\sin\gamma=2\cos\gamma — Young's fringes under an envelope
Grating limit, N→∞N\to\inftyprincipals →\to delta-like lines, R=mNR=mNideal grating; secondary maxima wash into a smooth background
Missing orders, d=qad=qam=q,2q,3q,…m=q,2q,3q,\dots extinguishedan envelope zero coincides with a principal maximum
Strongest secondary (large NN)4/(9π2)=4.5%4/(9\pi^2)=4.5\% of a principalsubsidiary lobes never rival the principal and shrink with NN

Worked examples

1 · Counting and sizing the ripples for six slits (confidence builder)

Six identical slits are ruled with spacing d=1666.67d=1666.67 nm and illuminated at normal incidence by λ=633\lambda=633 nm light. Locate the first principal maximum, state its height, and find how many secondary maxima lie between principals and how bright the strongest one is.

Step 1. The first principal is the grating equation with m=1m=1: sin⁡θ1=λ/d=633/1666.67=0.3798\sin\theta_1=\lambda/d=633/1666.67=0.3798, so θ1=arcsin⁡(0.3798)=22.32∘\theta_1=\arcsin(0.3798)=\mathbf{22.32^\circ} — the same order angle as a full grating of this pitch, because position depends only on dd.

Step 2. Its height is N2=62=36N^2=6^2=\mathbf{36} times the single-slit intensity in that direction. All six phasors align, so the amplitude is 66 and the intensity 3636.

Step 3. Between adjacent principals there are N−1=5N-1=\mathbf{5} zeros (at γ=pπ/6\gamma=p\pi/6, p=1,…,5p=1,\dots,5) and N−2=4N-2=\mathbf{4} secondary maxima. The strongest sits near Nγ=3π/2N\gamma=3\pi/2, i.e. γ≈π/4\gamma\approx\pi/4, where the array factor is 2.062.06; dividing by 3636 gives 5.7%\mathbf{5.7\%} of the principal.

Step 4. Compare the discredited textbook formula N2/(1+N2)=36/37=0.973N^2/(1+N^2)=36/37=0.973, which would put the ripple at 97%97\% of the line — seventeen times too high and qualitatively wrong. First principal at 22.32∘22.32^\circ, height 36×36\times; 55 zeros and 44 secondary maxima per gap, the strongest just 5.7%5.7\% of the principal.

2 · What happens as the grating grows (exam level)

Keep the same pitch and wavelength but increase the number of illuminated slits from 66 to 2020 to 3000030000 (a 5050 mm grating at 600600 l/mm). Track the strongest secondary maximum and the width and resolving power of the first-order line.

Step 1. The strongest secondary maximum falls with NN: from 5.7%5.7\% at N=6N=6 to 4.8%\mathbf{4.8\%} at N=20N=20, settling to a few percent, with the standard large-NN estimate 4/(9π2)=4.5%4/(9\pi^2)=\mathbf{4.5\%}. The ripples do not vanish, but they sink into a smooth, faint background relative to ever-brighter lines.

Step 2. The first-order line sharpens as 1/N1/N. Its angular half-width is Δθ1/2=λ/(Ndcos⁡θ1)\Delta\theta_{1/2}=\lambda/(Nd\cos\theta_1); with Nd=30000×1666.67Nd=30000\times1666.67 nm =50=50 mm and cos⁡θ1=0.925\cos\theta_1=0.925, this is 633×10−9/(0.050×0.925)=1.37×10−5633\times10^{-9}/(0.050\times0.925)=1.37\times10^{-5} rad =13.7 μrad=\mathbf{13.7\ \mu\text{rad}}.

Step 3. The resolving power is R=mN=1×30000=30000R=mN=1\times30000=\mathbf{30000}, so at 589589 nm it separates wavelengths differing by Δλ=λ/R=19.6\Delta\lambda=\lambda/R=19.6 pm — enough to split the sodium D-doublet (0.60.6 nm) roughly thirty times over. Secondaries fade from 5.7%→4.8%→4.5%5.7\%\to4.8\%\to4.5\%; the line narrows to 13.7 μrad13.7\ \mu\text{rad} and resolves R=mN=30000R=mN=30000.

Physics of the portrait

The portrait of this article is not a person but an operation — the Fourier transform — because the NN-slit pattern is not merely described by a transform, it is one.

Origins · 1 minfourier transform and how this was discovered
FT
fourier transform
the far field is the transform of the aperture · Fourier optics and diffraction

The Fourier transform decomposes any function into its sinusoidal components, and in the Fraunhofer regime it is the machine that turns an aperture into its diffraction pattern: each observation direction reads off one spatial-frequency component of the opening. The NN-slit array is the cleanest demonstration. Its aperture is a single rectangle convolved with a comb of NN points, and because the transform sends convolution to multiplication, the pattern is forced to be a product — a sinc\mathrm{sinc} envelope from the rectangle times an array factor from the comb. The transform's operations become physical facts: a slit and its diffraction envelope have reciprocal widths (narrow slit, broad envelope), and the more periods you illuminate the sharper the transform of the comb, which is why resolving power grows as NN. The mathematics descends from Joseph Fourier, who introduced his series and integral to solve the flow of heat and, in doing so, handed optics the language it now speaks natively — a lens and a distance do to light exactly what the transform does to a function.

History
1807
— Joseph Fourier presents his theory of heat to the Paris Institute, introducing the decomposition into sinusoids that becomes the Fourier transform
1821
— Joseph von Fraunhofer formulates the far-field theory of the diffraction grating
1822
— Fourier's Théorie analytique de la chaleur lays out the transform in full
1835
— Friedrich Magnus Schwerd works out the quantitative multiple-slit diffraction pattern
1874
— Lord Rayleigh derives the grating's chromatic resolving power, R=mNR=mN

Going further

Texts. Hecht, Optics, 5th ed., §10.2 (Fraunhofer diffraction: the many-slit pattern and the grating) · Foot, Atomic Physics, §A.2 (diffraction gratings and resolving power) · Saleh & Teich, Fundamentals of Photonics, 3rd ed., Ch. 4 (Fourier optics of periodic apertures) · Goodman, Introduction to Fourier Optics, 4th ed., Ch. 4 · Demtröder, Laser Spectroscopy, Vol. 1 (grating spectrometers and resolution). Key checkpoints for the core results: (i) the geometric-series sum giving [sin⁡Nγ/sin⁡γ]2[\sin N\gamma/\sin\gamma]^2; (ii) the N=1,2N=1,2 limits (sin⁡2γ/sin⁡γ=2cos⁡γ\sin2\gamma/\sin\gamma=2\cos\gamma); (iii) the peak value N2N^2 at γ→mπ\gamma\to m\pi; (iv) the first-zero half-width γ=π/N\gamma=\pi/N and hence Δθ=λ/(Ndcos⁡θm)\Delta\theta=\lambda/(Nd\cos\theta_m); (v) R=mNR=mN by combining dispersion with the Rayleigh criterion; and (vi) missing orders when d/ad/a is integer. The illustrative numbers R=2000R=2000 and 0.250.25 nm are standard textbook values.

Provenance addendum (correction). The source material's secondary-maximum formula, Isec≈N2/(1+(N/π)2π2)=N2/(1+N2)→1I_{\text{sec}}\approx N^2/(1+(N/\pi)^2\pi^2)=N^2/(1+N^2)\to1, is physically wrong: a secondary lobe cannot approach the principal. This article corrects it to the standard result — the strongest secondary maximum is only a few percent of the principal: the exact maxima are 0.05720.0572 (N=6N=6) and 0.04800.0480 (N=20N=20), and the standard large-NN estimate, taking the secondary at Nγ=3π/2N\gamma=3\pi/2, is 4/(9π2)=0.04504/(9\pi^2)=0.0450.

Prerequisites. Fraunhofer Diffraction · Single-Slit Diffraction · Huygens–Fresnel Principle · Fresnel Number. Leads to. Grating Equation · Grating Resolving Power and Dispersion · Rayleigh Resolution Criterion.

Why do the principal maxima get sharper as I add more slits?

Because the first zero moves closer to the peak. A principal is flanked by a zero a phase π/N\pi/N away in γ\gamma, so its angular half-width is λ/(Ndcos⁡θ)\lambda/(Nd\cos\theta) — inversely proportional to the total illuminated width NdNd. Killing a maximum only needs the extreme slits to drift half a wavelength out of step, and with more slits that misalignment builds over a smaller tilt. So doubling the slit count halves the line width while raising the peak fourfold — why a grating with tens of thousands of lines resolves doublets a two-slit interferometer never could.

If the peak intensity is N² times a single slit, where does all that energy come from?

It is redistributed, not created. The single-slit envelope fixes how much light leaves each slit in a direction; adding slits does not change the total power, only where it lands. At a principal the NN contributions add in phase, giving amplitude NN and intensity N2N^2 — but the peak is only 1/N1/N as wide, so the energy under it scales as N2×(1/N)=NN^2\times(1/N)=N, matching the NN slits' share. Between principals the light is removed by destructive interference and piled into the lines. Energy is conserved; interference merely concentrates it.

What exactly was wrong with the secondary-maximum formula this article corrects?

The formula Isec≈N2/(1+(N/π)2π2)I_{\text{sec}}\approx N^2/(1+(N/\pi)^2\pi^2) simplifies to N2/(1+N2)→1N^2/(1+N^2)\to1 — it claims the brightest ripple is almost as tall as a grating line. That cannot happen: a principal reaches N2N^2 because all phasors align, whereas a secondary lives where they nearly cancel. The exact strongest secondary is a few percent — 5.7%5.7\% at N=6N=6, 4.8%4.8\% at N=20N=20 — and the standard large-NN estimate is 4/(9π2)=4.5%4/(9\pi^2)=4.5\%, from the array factor at Nγ=3π/2N\gamma=3\pi/2. The trend is opposite too: the true ratio decreases with NN, while the bad formula rises toward 11.

How is this different from Young's two-slit interference?

It is the same physics with more sources, and N=2N=2 is a special case. Setting N=2N=2 gives [sin⁡2γ/sin⁡γ]2=4cos⁡2γ[\sin2\gamma/\sin\gamma]^2=4\cos^2\gamma, the familiar cosine-squared fringes under the single-slit envelope. What changes as NN grows is sharpness: two slits give broad, equally spaced maxima with nothing between them; many slits give narrow lines (width ∝1/N\propto1/N) separated by dark gaps with only faint secondary ripples. The maxima stay put — fixed by dsin⁡θ=mλd\sin\theta=m\lambda — but become far sharper and taller.

Does the single-slit envelope shift the positions of the principal maxima?

No. The envelope and array factor depend on different lengths and act independently: the principal positions are set entirely by the spacing dd through dsin⁡θ=mλd\sin\theta=m\lambda, while the envelope, set by the width aa, only scales the brightness at each fixed angle. The envelope can dim an order, or extinguish it if one of its zeros (asin⁡θ=pλa\sin\theta=p\lambda) lands on a principal — the missing-order case — but it never moves a maximum. This clean split of position from brightness is exactly what the convolution/Fourier picture guarantees.

Why is the far-field pattern of N slits a Fourier transform at all?

Because in the Fraunhofer regime each direction collects wavelets that left the aperture along parallel rays, so their only relative phase is linear in position — and summing linear-phase contributions across the aperture is the definition of a Fourier transform. The aperture and its far field form a transform pair, with angle as spatial frequency u=sin⁡θ/λu=\sin\theta/\lambda. For NN slits the aperture is a rectangle convolved with a comb, so its transform is a product of a sinc and an array factor. It is the same reason a lens, which brings the far field to its focal plane, is called an analog Fourier-transform engine.

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