The Diffraction Grating (AQA AS Physics)

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Katie M

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The Diffraction Grating

  • A diffraction grating is a piece of optical equipment that also creates a diffraction pattern when it diffracts:
    • Monochromatic light into bright and dark fringes
    • White light into its different wavelength components

Diffraction grating diagram, downloadable AS & A Level Physics revision notes

Diagram of diffraction grating used to obtain a fringe pattern

  • A diffraction grating consists of a large number of very thin, equally spaced parallel slits carved into a glass plate

The Diffraction Grating Equation

  • Diffraction gratings are useful because they create a sharper pattern than a double slit

    • This means their bright fringes are narrower and brighter while their dark regions are wider and darker

  • Just like for single and double-slit diffraction the regions where constructive interference occurs are also the regions of maximum intensity
  • Their location can be calculated using the diffraction grating equation

Grating equation, downloadable AS & A Level Physics revision notes

  • Where:
    • n is the order of the maxima, the number of the maxima away from the central (= 0)
    • d is the distance between the slits on the grating (m)
    • θ is the angle of diffraction of the light of order n from the normal as it leaves the diffraction grating (°)
    • λ is the wavelength of the light from the source (m)

Slit Spacing

  • Diffraction gratings come in different sizes
    • The sizes are determined by the number of lines per millimetre (lines / mm) or lines per m
    • This is represented by the symbol N
  • d can be calculated from N using the equation
    • If is given in terms of lines per mm then will be in mm
    • If is given in terms of lines per m then will be in m

Angular Separation

  • The angular separation of each maxima is calculated by rearranging the grating equation to make θ the subject
  • The angle θ is taken from the centre meaning the higher orders of n are at greater angles

Angular separation, downloadable AS & A Level Physics revision notes

Angular separation increases as the order of maxima increases

  • The angular separation between two angles is found by subtracting the smaller angle from the larger one
  • The angular separation between the first and second maxima at n1 and n2 is θ2θ1

Orders of Maxima

  • The maximum angle of diffraction with which maxima can be seen is when the beam is at right angles to the diffraction grating
    • This means θ = 90o and sin θ = 1

  • The highest order of maxima visible is therefore calculated by the equation:

  • Since n is an integer number of maxima, if the value obtained is a decimal it must be rounded down to determine the highest-order visible
    • E.g If n is calculated as 2.7 then n = 2 is the highest-order visible

Worked example

An experiment was set up to investigate light passing through a diffraction grating with a slit spacing of 1.7 µm. The fringe pattern was observed on a screen. The wavelength of the light is 550 nm.Worked Example: Diffraction Grating, downloadable AS & A Level Physics revision notes

Calculate the angle α between the two second-order lines.

Worked example - diffraction grating equation (2), downloadable AS & A Level Physics revision notes

Exam Tip

Take care that the angle θ is the correct angle taken from the centre and not the angle taken between two orders of maxima.

Derivation of the Diffraction Grating Equation

  • When light passes through the slits of the diffraction grating, the path difference at the zeroth order maximum is zero
  • At the first order maxima, there is constructive interference, hence the path difference is λ
  • Therefore, at the nth order maxima, the path difference is equal to nλ

Diffraction Grating Equation, downloadable AS & A Level Physics revision notes

Using this diagram and trigonometry, the diffraction grating equation can be derived

  • Using trigonometry, an expression for the first order maxima can be written:

  • Where:
    • θ = the angle between the normal and the maxima
    • λ = the wavelength of the light (m)
    • d = the slit separation (m)

  • This means, for n = 1:

  • Similarly, for n = 2, where the path difference is 2λ:

  • Therefore, in general, where the path difference is nλ:

  • A small rearrangement leads to the equation for the diffraction grating:

d sin θn = nλ

Applications of Diffraction Gratings

  • Diffraction gratings are useful for separating light of different wavelengths with high-resolution
  • They are used in spectrometers to:
    • Analyse light from stars
    • Analyse the composition of a star
    • Chemical analysis
    • Measure red shift / rotation of stars
    • Measure the wavelength / frequency of light from a star
    • Observe the spectra of materials
    • Analyse the absorption / emission spectra in stars

  • Diffraction gratings also play a role in X-ray crystallography:
    • X-rays are directed at a thin crystal sheet which acts as a diffraction grating to form a diffraction pattern
    • This is because the wavelength of X-rays is similar in size to the gaps between the atoms
    • This diffraction pattern can be used to measure the atomic spacing in certain materials

  • Diffraction gratings are also used in monochromators:
    • To specifically analyse a wavelength emitted by molecules in diseased cells from a biopsy sample
    • To help excite molecules in a sample with a specific wavelength of light
  • Diffraction gratings are used to select the optimum wavelength of light for use in an optical fibre

Diffraction Grating Applications, downloadable AS & A Level Physics revision notes

Diffraction gratings are most commonly used in spectrometers. These devices play a crucial role in areas of physics such as atomic physics and astrophysics

Exam Tip

Note that while you will be expected to know some applications of diffraction gratings, you will not be tested on specific apparatus or techniques such as spectrometry.When describing the use of spectrometers, avoiding using vague terms such as observe spectra’, ‘spectroscopy’, ‘view absorption / emission spectrum’, ‘compare spectra’, ‘look at light from stars’.

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Katie M

Author: Katie M

Katie has always been passionate about the sciences, and completed a degree in Astrophysics at Sheffield University. She decided that she wanted to inspire other young people, so moved to Bristol to complete a PGCE in Secondary Science. She particularly loves creating fun and absorbing materials to help students achieve their exam potential.