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4.4 Diffraction Gratings

Thousands of lines per centimeter spreading wavelengths into sharp, widely separated orders, the basis of spectrometers reading atomic emission.

University Physics Volume 3, 4.4 Diffraction Gratings

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7 exercises

4.4 Exercise 1

If the line spacing of a diffraction grating d is not precisely known, we can use a light source with a well-determined wavelength to measure it. Suppose the first-order constructive fringe of the Hβ\text{H}_{\beta} emission line of hydrogen (λ=656.3nm)\left(\lambda = 656.3 \text{nm}\right) is measured at 11.36°11.36 ° using a spectrometer with a diffraction grating. What is the line spacing of this grating?

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4.4 Exercise 2

A diffraction grating has 2000 lines per centimeter. At what angle will the first-order maximum be for 520-nm-wavelength green light?

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4.4 Exercise 4

How many lines per centimeter are there on a diffraction grating that gives a first-order maximum for 470-nm blue light at an angle of 25.0°25.0 ° ?

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4.4 Exercise 6

Calculate the wavelength of light that has its second-order maximum at 45.0°45.0 ° when falling on a diffraction grating that has 5000 lines per centimeter.

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4.4 Exercise 8

(a) What do the four angles in the preceding problem become if a 5000-line per centimeter diffraction grating is used? (b) Using this grating, what would the angles be for the second-order maxima? (c) Discuss the relationship between integral reductions in lines per centimeter and the new angles of various order maxima.

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4.4 Exercise 10

An opal such as that shown in the figure acts like a reflection grating with rows separated by about 8μm.8 \mu\text{m} . If the opal is illuminated normally, (a) at what angle will red light be seen and (b) at what angle will blue light be seen?

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4.4 Exercise 12

(a) Find the maximum number of lines per centimeter a diffraction grating can have and produce a maximum for the smallest wavelength of visible light. (b) Would such a grating be useful for ultraviolet spectra? (c) For infrared spectra?

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Adapted from University Physics Volume 3 © 2016 Rice University. Licensed under CC BY 4.0. Source: University Physics Volume 3. Imported at revision db44eb9.