Gratings: Dispersion and Resolving Power — Question 1

Section 36-8 · Physics pages 5992–5993

Question 1 Differentiating the grating equation gives angular dispersion A normally illuminated grating obeys d sin θ = mλ. Let d = 2.00 µm, order m=2, and central wavelength 500 nm. d N illuminated slits Schematic; labels, not drawing lengths, specify the data. (a) Derive and evaluate angular dispersion D = dθ/dλ at this wavelength. (b) Estimate the angular separation of two lines differing by 2.00 nm.
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Question 1 - Solution Differentiating the grating equation gives angular dispersion d N illuminated slits (a) Method and calculation d cos θ dθ = m dλ =⇒D = m d cos θ . sin θ = 0.500 =⇒θ = 30◦, D = 1.15470 × 106 rad/m . (b) Interpretation and further calculation D = 1.15470 mrad/nm. ∆θ ≃D∆λ = 2.30940 mrad . Physical check The derivative is a local linear approximation; finite wavelength intervals require the inverse-sine grating equation if higher accuracy is needed.

Question 1

Differentiating the grating equation gives angular dispersion

A normally illuminated grating obeys dsin⁡θ=mλd\sin\theta=m\lambda. Let d=2.00μmd=2.00\,\mu\mathrm m, order m=2, and central wavelength 500nm500\,\mathrm{nm}.

Diagram shown in the original SVG worksheet.

  1. Derive and evaluate angular dispersion 𝒟=dθ/dλ\mathcal D=d\theta/d\lambda at this wavelength.

  2. Estimate the angular separation of two lines differing by 2.00nm2.00\,\mathrm{nm}.

Question 1 - Solution

Differentiating the grating equation gives angular dispersion

Diagram shown in the original SVG worksheet.

(a) Method and calculation

dcos⁡θdθ=mdλ⇒𝒟=mdcos⁡θ.d\cos\theta\,d\theta=m\,d\lambda\Longrightarrow\boxed{\mathcal D=\frac m{d\cos\theta}}.sin⁡θ=0.500⇒θ=30∘,𝒟=1.15470×106rad/m.\sin\theta=0.500\Longrightarrow\boxed{\theta=30^\circ,\quad\mathcal D=1.15470\times10^6\,\mathrm{rad/m}}.

(b) Interpretation and further calculation

𝒟=1.15470mrad/nm.\mathcal D=1.15470\,\mathrm{mrad/nm}.Δθ≃𝒟Δλ=2.30940mrad.\boxed{\Delta\theta\simeq\mathcal D\Delta\lambda=2.30940\,\mathrm{mrad}}.

Physical check

The derivative is a local linear approximation; finite wavelength intervals require the inverse-sine grating equation if higher accuracy is needed.