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Questions on diffraction gratings
A grating replaces two slits with thousands, and its maxima are sharper and brighter because the light from every slit has to arrive in step. The grating equation d sin θ = nλ locates each order, with d the slit spacing found from the number of lines per millimetre. A sine cannot exceed one, so only a few orders exist.
18 original questions · 58 marks · the diffraction gratings notes · Waves
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State the diffraction grating equation and define each term in it.
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d sinθ = nλ (1), where d is the grating spacing, the distance between adjacent slits, θ the angle of the maximum, n the order, and λ the wavelength (1).A diffraction grating has 300 lines per millimetre. Calculate the grating spacing d in metres.
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d = 1/(300 × 103 lines per metre) (1)
d = 3.33 × 10−6 m (1)Explain why a diffraction grating produces sharper, brighter maxima than a double slit.
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A grating has many slits, so far more beams interfere (1). Constructive interference occurs only at precise angles where all beams are in phase, giving narrow, intense maxima; away from these angles the many beams cancel (1).State what is meant by the zero-order maximum produced by a diffraction grating, and give the path difference between light from adjacent slits at this maximum.
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The maximum in the straight-through direction, along the normal to the grating (n = 0) (1). The path difference between light from adjacent slits there is zero (1).Explain why, for a given grating and wavelength, only a limited number of orders of maxima can be produced.
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The grating equation gives sinθ = nλ/d, and sinθ cannot exceed 1 (1). Orders therefore exist only while nλ/d ≤ 1, so no order beyond the whole-number part of d/λ has an angle at which it can form (1).Light of wavelength 600 nm is shone normally at a grating with 500 lines per millimetre. Calculate the angle of the first-order maximum.
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d = 1/(500 × 103) (1)
d = 2.00 × 10−6 m (1)
sinθ = nλ/d = (1 × 600 × 10−9)/(2.00 × 10−6) (1)
θ = 17.5° (1)Light of wavelength 600 nm is incident normally on a grating with 500 lines per millimetre. Calculate the angle of the second-order maximum.
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d = 1/(500 × 103) = 2.00 × 10−6 m (1)
sinθ = 2λ/d = (2 × 600 × 10−9)/(2.00 × 10−6) (1)
θ = 36.9° (1)A grating with 600 lines per millimetre gives a first-order maximum at 21°. Calculate the wavelength of the light.
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d = 1/(600 × 103) = 1.67 × 10−6 m (1)
λ = d sinθ = 1.67 × 10−6 × sin 21° (1)
λ = 597 nm (1)Light of wavelength 500 nm gives a first-order maximum at 15° with a certain grating. Calculate the grating spacing and hence the number of lines per millimetre.
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d = λ/sinθ = (500 × 10−9)/sin 15° (1)
d = 1.93 × 10−6 m (1)
Lines per mm = 1/d per metre ÷ 1000 = 518 lines per mm (1)Blue light of wavelength 486 nm from a hydrogen discharge lamp is incident normally on a grating with 420 lines per millimetre. Show that the grating spacing is about 2.4 × 10−6 m. Go on to calculate the angle of the third-order maximum.
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d = 1/(420 × 103 lines per metre) (1) = 2.38 × 10−6 m ≈ 2.4 × 10−6 m (1). sinθ = 3λ/d = (3 × 486 × 10−9)/(2.38 × 10−6) = 0.612 (1), so θ = 37.8° (allow 37.4° to 37.8°) (1).A laser of wavelength 633 nm shines normally through a grating with 250 lines per millimetre. The maxima form spots on a screen 1.5 m beyond the grating and parallel to it. Calculate the distance on the screen between the two first-order spots.
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d = 1/(250 × 103) = 4.00 × 10−6 m (1). sinθ = λ/d = (633 × 10−9)/(4.00 × 10−6), so θ = 9.1° (1). Distance of each spot from the centre x = 1.5 × tanθ = 0.24 m (1). Separation of the two first-order spots = 2x = 0.48 m (1).To reduce the uncertainty in an angle measurement, a student measures the angle between the two first-order maxima on either side of the centre and obtains 40.0°. The grating has 600 lines per millimetre. Calculate the wavelength of the light.
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First-order angle from the centre θ = 40.0°/2 = 20.0° (1). λ = d sinθ = 1.67 × 10−6 × sin 20.0° (1) = 5.70 × 10−7 m = 570 nm (1).A grating has a spacing of 2.0 × 10−6 m and is used with 600 nm light. Calculate the highest order of maximum that can be seen, and the angle at which it appears.
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The maximum order is where sinθ = 1, so nmax = d/λ (1)
= (2.0 × 10−6)/(600 × 10−9) = 3.33 (1)
The highest order is therefore n = 3 (1)
At that order sinθ = 3 × 600 × 10−9/(2.0 × 10−6), giving θ = 64.2° (1)White light (400 nm to 700 nm) passes normally through a grating of spacing 2.0 × 10−6 m. Calculate the angular width of the first-order spectrum (the angle between the 400 nm and 700 nm maxima).
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First order: sinθ = λ/d (1)
For 400 nm, θ = 11.5° (1)
For 700 nm, θ = 20.5° (1)
Angular width = 9.0°, with red diffracted more than violet (1)Give two practical uses of diffraction gratings.
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1. Measuring the wavelength of light or analysing spectra in a spectrometer (1). 2. Identifying elements from their line spectra, for example in the light from stars (1).White light with wavelengths from 400 nm to 700 nm passes normally through a grating with 400 lines per millimetre. Deduce whether the second-order and third-order spectra overlap.
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d = 1/(400 × 103) = 2.5 × 10−6 m (1). Red end of the second order: sinθ = (2 × 700 × 10−9)/d = 0.56, so θ = 34.1° (1). Violet end of the third order: sinθ = (3 × 400 × 10−9)/d = 0.48, so θ = 28.7° (1). The third order begins at a smaller angle than the angle at which the second order ends, so the two spectra overlap (1).A teacher wants to show a class at least three orders of maxima on each side of the centre, using light of wavelength 589 nm from a sodium lamp. Two gratings are available: grating X with 300 lines per millimetre and grating Y with 800 lines per millimetre. Deduce which grating the teacher should use.
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Highest order = whole-number part of d/λ (1). Grating X: d = 3.33 × 10−6 m, d/λ = 5.66, so 5 orders are visible each side (1). Grating Y: d = 1.25 × 10−6 m, d/λ = 2.12, so only 2 orders are visible (1). Only X gives at least three orders, so the teacher should use grating X (1).White light with wavelengths from 400 nm to 700 nm is incident normally on a diffraction grating with 500 lines per millimetre. Describe and explain the appearance of the pattern produced, up to and including the second order, and show that the second-order spectrum is complete.
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The central (zero-order) maximum is white, because at n = 0 the path difference is zero for every wavelength, so all colours arrive in phase there (1). Each non-zero order is drawn out into a continuous spectrum with violet nearest the centre and red furthest out (1), because sinθ = nλ/d, so the angle of a maximum increases with wavelength (1). d = 1/(500 × 103) = 2.0 × 10−6 m, and the most demanding maximum is red in the second order: sinθ = (2 × 700 × 10−9)/(2.0 × 10−6) = 0.70, which is below 1, so the second-order spectrum runs the whole way to the red end (1). The first order spans 11.5° to 20.5° and the second 23.6° to 44.4°, so with this grating the two do not overlap (1). The second-order spectrum is the wider of the two and lies further from the centre, since doubling n doubles sinθ for every wavelength (1).
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