How does a diffraction grating separate light into sharp, well-resolved spectral lines?
Apply the diffraction grating equation to analyse the dispersion of light into spectra
A focused answer to the WACE Year 12 Physics Unit 4 content point on diffraction gratings. The grating equation, why many slits give sharp bright maxima, how a grating disperses white light into a spectrum, and finding wavelengths from the diffraction angle.
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What this dot point is asking
WACE wants you to use the grating equation, understand why many slits sharpen the maxima, and explain how a grating produces a spectrum. The grating is the precision instrument of wave optics.
The grating equation
For a grating with slit spacing (the distance between adjacent slits), bright maxima occur where
Here is the order of the maximum. The slit spacing is usually given as lines per millimetre , so in millimetres, which you convert to metres. The zeroth order () is straight through; higher orders appear at larger angles.
Why many slits give sharp lines
With only two slits the bright fringes are broad and gradually fade. With thousands of slits, light from all of them must be in phase to give a maximum, which happens only at very precise angles. A tiny deviation from the exact angle causes waves from different parts of the grating to cancel, so the maxima become extremely narrow and bright. This sharpness is what makes gratings able to resolve closely spaced wavelengths.
Dispersing light into a spectrum
Because the diffraction angle depends on wavelength, each colour in white light emerges at a slightly different angle in each order. The result is a spectrum spread out by wavelength, with violet (short wavelength) deviated least and red (long wavelength) most. Unlike a prism, a grating spreads the colours in a predictable, calculable way, which is why gratings are used in spectrometers to measure the wavelengths emitted by light sources.
Limits on the orders
Since cannot exceed , only a finite number of orders exist for a given grating and wavelength. The highest visible order is the largest integer for which . Long wavelengths and finely ruled gratings (small ) produce fewer orders.
Working with line densities
Convert lines per millimetre to a spacing in metres before substituting, and remember must be a whole number. If a calculation gives for some order, that order does not exist for that wavelength.