Convolution and a finite slit array

ID: past-exam-of-the-physics-a-course-of-the-university-of-cambridge/2017/paper-2/section-b/b8/convolution-and-a-finite-slit-array

Use Fourier transform convention . The convolution theorem gives
A finite array of very narrow slits at , , has transmission proportional to . It can be constructed by multiplying an infinite Dirac comb by a finite window. The infinite comb transforms to a reciprocal comb; the finite window convolves each reciprocal peak with a narrow sinc-shaped amplitude. Thus increasing the illuminated length narrows each Fraunhofer diffraction peak.
The exact finite sum makes the argument quantitative:
Its normalized intensity is . Principal maxima occur at ; their first zeros are displaced by . Replacing the ideal narrow slit by a finite slit function convolves the array in real space, multiplying this field by the single-slit Fourier transform. Field amplitudes are transformed and combined before their squared modulus is taken.
Figure 1.
A finite narrow-slit array and its Fourier intensity, showing how the principal peaks narrow with slit count
. Details.

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