Required Practical: Young's Slit Experiment & Diffraction Gratings (AQA A Level Physics): Revision Note

Required practical: Young's slit experiment & diffraction gratings

Equipment list

• Resolution of measuring equipment:

  • Metre ruler = ±1 mm

  • Vernier Callipers = ±0.01 mm

Young’s double-slit experiment

The overall aim of this experiment is to investigate the relationship between the slit-screen distance, $D$, and the fringe width, $w$

• Independent variable = Distance between the slits and the screen, $D$

• Dependent variable = Fringe width, $w$

• Control variables:

  • Wavelength of laser light, $\lambda$

  • Slit separation, $s$

Method

1. Set up the apparatus by fixing the laser and the slits to a retort stand and place the screen so that $D$ is 0.5 m, measured using the metre ruler.

2. Darken the room and turn on the laser.

3. Measure from the central fringe across many fringes using the vernier callipers and divide by the number of fringe widths to find the fringe width, $w$.

4. Increase the distance $D$ by 0.1 m and repeat the procedure, increasing it by 0.1 m each time up to around 1.5 m.

5. Repeat the experiment twice more and calculate and record the mean fringe width $w$ for each distance $D$.

• An example table might look like this:

Analysing the results

• The fringe spacing equation is given by:

$w=\frac{\lambda D}{s}$

• Where:

  • $w$ = the distance between each fringe (m)

  • $\lambda$ = the wavelength of the laser light (m)

  • $D$ = the distance between the slit and the screen (m)

  • $s$ = the slit separation (m)

• Comparing this to the equation of a straight line: $y=mx$

  • $y=w$ (m)

  • $x=D$ (m)

  • Gradient $=\frac{\lambda }{s}$ (unitless)

• Plot a graph of $w$ against $D$ and draw a line of best fit

• The wavelength of the laser light is equal to the gradient multiplied by the slit separation, because:

Interference by a diffraction grating

The overall aim of this experiment is to calculate the wavelength of the laser light using a diffraction grating

• Information on how a diffraction grating works can be found in the revision note 3.4.2 The Diffraction Grating

• Independent variable = Distance between maxima, $h$

• Dependent variable = The angle between the normal and each order, ${\theta }_n$ (where n = 1, 2, 3 etc)

• Control variables:

  • Distance between the slits and the screen, $D$

  • Laser wavelength, $\lambda$

  • Slit separation, $d$

Method

1. Place the laser on a retort stand and the diffraction grating in front of it.

2. Use a set square to ensure the beam passes through the grating at normal incidence and meets the screen perpendicularly.

3. Set the distance $D$ between the grating and the screen to be 1.0 m using a metre ruler.

4. Darken the room and turn on the laser.

5. Identify the zero-order maximum (the central beam).

6. Measure the distance $h$ to the two nearest first-order maxima (i.e. n = 1, n = 2) using a vernier calliper.

7. Calculate the mean of these two values.

8. Measure distance $h$ for increasing orders.

9. Repeat with a diffraction grating that has a different number of slits per mm.

• An example table might look like this:

Analysing the results

The diffraction grating equation is given by:

$n\lambda =d\sin \theta$

• Where:

  • $n$ = the order of the diffraction pattern

  • $\lambda$ = the wavelength of the laser light (m)

  • $d$ = the distance between the slits (m)

  • $\theta$ = the angle between the normal and the maxima

• The distance between the slits is equal to:

$d=\frac{1}{N}$

• Where:

  • $N$ = the number of slits per metre (m^–1)

• Since the angle is not small, it must be calculated using trigonometry with the measurements for the distance between maxima, $h$, and the distance between the slits and the screen, $D$

$\tan \theta =\frac{h}{D}$

$\theta ={\tan }^{-1}\left(\frac{h}{D}\right)$

• Calculate a mean $\theta$ value for each order

• Calculate a mean value for the wavelength of the laser light and compare the value with the accepted wavelength

  • This is usually 635 nm for a standard school red laser

Evaluating the experiments

• Systematic errors:

  • Ensure the use of the set square to avoid parallax error in the measurement of the fringe width

  • Using a grating with more lines per mm will result in greater values of $h$ — this lowers its percentage uncertainty

  • Measure the distance between each bright fringe from the centre of each bright spot

• Random errors:

  • The fringe spacing can be subjective depending on its intensity on the screen, therefore, take multiple measurements of $w$ and $h$ (between three and eight) and find the average

  • Use a Vernier scale to record distances $w$ and $h$ to reduce percentage uncertainty

  • Reduce the uncertainty in $w$ and $h$ by measuring across all visible fringes and dividing by the number of fringes

  • Increase the grating to screen distance $D$ to increase the fringe separation (although this may decrease the intensity of light reaching the screen)

  • Conduct the experiment in a darkened room, so the fringes are clear

Safety considerations

• Lasers should be Class 2 and have a maximum output of no more than 1 mW

• Do not allow laser beams to shine into anyone’s eyes

• Remove reflective surfaces from the room to ensure no laser light is reflected into anyone’s eyes