Required Practical: Inverse Square-Law for Gamma Radiation (AQA A Level Physics)

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Required Practical: Inverse Square-Law for Gamma Radiation

Aim of the Experiment

  • The aim of this experiment is to verify the inverse square law for gamma radiation of a known gamma-emitting radioactive source

Variables

  • Independent variable = the distance between the source and detector, x (m)
  • Dependent variable = the count rate / activity of the source, C
  • Control variables
    • The time interval of each measurement
    • The same thickness of aluminium foil
    • The same gamma source
    • The same GM tube

Equipment List

Required Practical 12 Equipment List Table, downloadable AS & A Level Physics revision notes

  • Resolution of equipment:
    • Metre ruler = 1 mm
    • Stopwatch = 0.01 s

Method

Required Practical 12 Apparatus, downloadable AS & A Level Physics revision notes

Set up for inverse-square law investigation

  1. Measure the background radiation using a Geiger Muller tube without the gamma source in the room, take several readings and find an average
  2. Next, put the gamma source at a set starting distance (e.g. 5 cm) from the GM tube and measure the number of counts in 60 seconds
  3. Record 3 measurements for each distance and take an average
  4. Repeat this for several distances going up in 5 cm intervals

  • A suitable table of results might look like this:

Required Practical 12 Data Example, downloadable AS & A Level Physics revision notes

Analysing the Results

  • According to the inverse square law, the intensity, I, of the gamma radiation from a point source depends on the distance, x, from the source

I space proportional to space 1 over x squared

  • Intensity is proportional to the corrected count rate, C, so:

C space proportional to space 1 over x squared

  • Rearranging this equation gives:

fraction numerator 1 over denominator square root of C end fraction space proportional to space x

fraction numerator 1 over denominator square root of C end fraction space equals space k x

  • Comparing this to the equation of a straight line, y = mx
    • y = fraction numerator 1 over denominator square root of C end fraction
    • x = x (m)
    • Gradient = constant, k

  1. Subtract the background radiation from each count rate reading to give the corrected count rate, C
  2. Plot a graph of fraction numerator 1 over denominator square root of C end fraction against distance x
  3. If it is a straight-line graph, this shows they are directly proportional, and the inverse square relationship is confirmed

Graph for Inverse Square Law Experiment

8-1-required-practical-gamma-inverse-square-law-graph

A straight-line graph verifies the inverse square relationship. If the line does not go through the origin, this indicates the presence of a systematic error in the measurement of distance

Evaluating the Experiment

Systematic errors:

  • The main source of systematic error in this experiment is in the measurement of distance
    • It is unlikely that the source is at the end of the tube, and it is unlikely that the detector is at the end of the GM tube
    • This means the measured distance is likely to be smaller than the actual distance
    • By plotting a graph of fraction numerator 1 over denominator square root of C end fraction against x, this discrepancy can be easily read off the graph where the line meets the negative x-axis

lHIsojDR_8-1-systematic-error-in-inverse-square-law-experiment

The exact positions of the gamma source and the detector in their sealed tubes are not known, so this gives rise to a systematic error in the measurement of distance

  • The Geiger counter may suffer from an issue called “dead time”
    • This is when multiple counts happen simultaneously within ~100 μs and the counter only registers one
    • This is a more common problem in older detectors, so using a more modern Geiger counter should reduce this problem
  • The source may not be a pure gamma emitter
    • To prevent any alpha or beta radiation from being measured, the Geiger-Muller tube should be shielded with a sheet of 2–3 mm aluminium
    • If alpha or beta emissions make it to the detector, this is likely to affect the shape of the graph, making it curve slightly

Random errors:

  • Radioactive decay is random, so repeat readings are vital in this experiment
  • Measure the count over the longest time span possible
    • A larger count helps reduce the statistical percentage uncertainty inherent in smaller readings
    • This is because the percentage error is proportional to the inverse-square root of the count

Safety Considerations

  • For the gamma source:
    • Reduce the exposure time by keeping it in a lead-lined box when not in use
    • Handle with long tongs
    • Do not point the source at anyone and keep a large distance (as activity reduces by an inverse square law)

  • Safety clothing such as a lab coat, gloves and goggles must be worn

Worked example

A student measures the background radiation count in a laboratory and obtains the following readings:

Required Practical 12 WE Table 1, downloadable AS & A Level Physics revision notes

The student is trying to verify the inverse square law of gamma radiation on a sample of Radium-226. He collects the following data:

Required Practical 12 WE Table 2, downloadable AS & A Level Physics revision notes

Use this data to determine:

(a)
if the student’s data follows an inverse square law
(b)
the uncertainty in the gradient of the graph.
 

Required Practical 12 Worked Example, downloadable AS & A Level Physics revision notes

Answer:

Part (a)

Step 1: Determine a mean value of background radiation

count space rate space equals space fraction numerator 69 space plus space 68 space plus space 70 space plus space 71 space plus space 69 space plus space 72 over denominator 6 end fraction space equals space 69.8 space equals space 70

Step 2: Calculate C (corrected average count rate) and C–1/2 

Required Practical 12 WE Table 3, downloadable AS & A Level Physics revision notes

 

Step 3: Plot a graph of C–1/2 against x and draw a line of best fit

Required Practical 12 Worked Example(1), downloadable AS & A Level Physics revision notes

  • The graph shows C–1/2 is directly proportional to x, therefore, the data follows an inverse square law

Part (b)

Step 1: Determine the uncertainties in the readings

  • Uncertainty in the count rate:  increment C space equals space 1 half cross times open parentheses range space of space repeat space readings close parentheses
  • Maximum value of C:  C subscript m a x end subscript space equals space C space plus space increment C
  • Error bars found from:  increment open parentheses fraction numerator 1 over denominator square root of C end fraction close parentheses space equals space fraction numerator 1 over denominator square root of C subscript m a x end subscript end root end fraction space minus space fraction numerator 1 over denominator square root of C end fraction

Required Practical 12 WE Table 4, downloadable AS & A Level Physics revision notes

Step 2: Plot the error bars and draw a line of worst fit

Required Practical 12 Worked Example(2), downloadable AS & A Level Physics revision notes

Step 3: Calculate the uncertainty in the gradient

best space gradient space equals space fraction numerator increment y over denominator increment x end fraction space equals space fraction numerator 400 space minus space 0 over denominator 90 space minus space 0.5 end fraction space equals space 4.47

worst space gradient space equals space fraction numerator increment y over denominator increment x end fraction space equals space fraction numerator 462 space minus space 0 over denominator 90 space minus space 7 end fraction space equals space 5.57

percent sign space uncertainty space equals space fraction numerator worst space gradient space minus space best space gradient over denominator best space gradient end fraction cross times 100 percent sign

percent sign space uncertainty space equals space fraction numerator 5.57 space minus space 4.47 over denominator 4.47 end fraction space cross times space 100 percent sign space equals space 24.6 percent sign

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Katie M

Author: Katie M

Expertise: Physics

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.