Diffraction Gratings — Question 1

Section 36-7 · Physics pages 5972–5973

Question 1 A finite grating is a geometric sum of equally rotated phasors N identical narrow slits contribute equal amplitudes E1eijδ, where j = 0, . . . , N −1 and δ = 2πd sin θ/λ. Ignore the slowly varying individual-slit envelope. d N illuminated slits Schematic; labels, not drawing lengths, specify the data. (a) Sum the phasors and derive the array intensity factor. (b) Evaluate the removable limit at a principal maximum and the peak increase if N doubles with each slit unchanged.
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Question 1 - Solution A finite grating is a geometric sum of equally rotated phasors d N illuminated slits (a) Method and calculation EN = E1 1 −eiNδ 1 −eiδ = E1ei(N−1)δ/2 sin(Nδ/2) sin(δ/2) . IN = I1 [sin(Nδ/2) sin(δ/2) ]2 . (b) Interpretation and further calculation δ →2πm : Iprincipal = N2I1 . N →2N =⇒Iprincipal →4Iprincipal . Physical check The zero-over-zero form at a principal order represents complete phase alignment rather than a dark direction.

Question 1

A finite grating is a geometric sum of equally rotated phasors

N identical narrow slits contribute equal amplitudes E1eijδE_1e^{ij\delta}, where j=0,…,N−1j=0,\ldots,N-1 and δ=2πdsin⁡θ/λ\delta=2\pi d\sin\theta/\lambda. Ignore the slowly varying individual-slit envelope.

Diagram shown in the original SVG worksheet.

  1. Sum the phasors and derive the array intensity factor.

  2. Evaluate the removable limit at a principal maximum and the peak increase if N doubles with each slit unchanged.

Question 1 - Solution

A finite grating is a geometric sum of equally rotated phasors

Diagram shown in the original SVG worksheet.

(a) Method and calculation

EN=E11−eiNδ1−eiδ=E1ei(N−1)δ/2sin⁡(Nδ/2)sin⁡(δ/2).E_N=E_1\frac{1-e^{iN\delta}}{1-e^{i\delta}}=E_1e^{i(N-1)\delta/2}\frac{\sin(N\delta/2)}{\sin(\delta/2)}.IN=I1[sin⁡(Nδ/2)sin⁡(δ/2)]2.\boxed{I_N=I_1\left[\frac{\sin(N\delta/2)}{\sin(\delta/2)}\right]^2}.

(b) Interpretation and further calculation

δ→2πm:Iprincipal=N2I1.\delta\to2\pi m:\quad\boxed{I_{\mathrm{principal}}=N^2I_1}.N→2N⇒Iprincipal→4Iprincipal.N\to2N\Longrightarrow\boxed{I_{\mathrm{principal}}\to4I_{\mathrm{principal}}}.

Physical check

The zero-over-zero form at a principal order represents complete phase alignment rather than a dark direction.