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Inverse square law for gamma radiation
Introduction

All forms of radiation follow the inverse square law.  That is the intensity of radiation declines as to the square of the distance from the source.  This can be mentally justified quite simply by considering the relative areas of concentric spheres.  The area of a sphere is given by:

 

    A = 4πR²

This tells us how the area of the ‘front’ expands from the origin.  If it needs to cover an area proportional to R2 then it is going to be weakened or attenuated by 1/R2 as the same amount of radiation now has to cover an area that has increased by a factor of R².

  • Question: What is the area that a light source illuminates after one millionth of second, two millionths of a second, three millionths through to 10 millionths.  Draw a graph of time on the x-axis against area on the y-axis.

Johannes Kepler, the astronomer, would appear to be the first to argue (in 1604) that the intensity of light from a source obeys the inverse square law.

Gamma rays are electromagnetic radiation, the same as light and radio waves, but at a high frequency, which means a high energy.  In fact, they are the highest frequency form of electromagnetic radiation observed.  They were first discovered by a French chemist called Paul Villard while investigating the radiation from the element radium.  It was our old stamp collecting friend Ernest Rutherford, who named them gamma rays.

In this experiment, we measure the background radiation and the count rates of gamma particles hitting a detector at a range of distances.  Plotting the results will verify the inverse square law. 

The objective

To show that gamma radiation follows the inverse square law in that the intensity falls off in proportion to one over the square of the distance from the source.

The apparatus

You will need:

  • Safe source of gamma radiation such as Cobalt 60;

  • Geiger counter;

  • 1 metre rule;

  • Thick lead block;

  • Stop watch.

 

Teachers, technicians and students must be aware of all regulations involved in handling radioactive substances.  Cobalt 60 is a common radioactive substance commonly used in this experiment and must be handled in accordance with these regulations.  Naturally, there are no safety concerns with using the e-practical.

This shows the electronic counter connected to the detector at the left. The radiation source is at the right, between the two is a ruler. Near the source is a large lead block.
The variables

The independent variable is the distance, and the dependent variable is the incident count rate.

The counter on the left counts the number of gamma rays hitting the detector that is to the right of it.  The counter and detector are connected by the cable.  To the right of the detector is a ruler.  At the far right is the gamma ray source.  There is also a large lead block that can be used to block the gamma rays.

The Physics

See the introduction above.

The method 

Start by moving the lead block between the ruler and the source as close to the source as possible. Start your timer at the same time as you press the start button on the electronic counter. Stop the counter at 20 minutes.

Now remove the lead block and move the source to 60 cm on the ruler. Count the particles for a 10-minute period. Repeat this for distances at 10-cm intervals down to 10 cm. You can time for less than 5 minutes where the counts are high. Do not forget to record the actual period length.

The Video

Watch a video for the Inverse Square Law e-practical here.

This shows how to use it and how to collect the data.

The E-Practical

 

Perform the experiment yourself, collect your own data, make mistakes and be able to correct them.  The e-practical requires that your browser can run WebGL 2 (usually found on Windows browsers, safari on iOS, and various Mobile browsers, test with https://get.webgl.org/webgl2/).  This link is for students and evaluation only, schools should purchase a site licence.

All the e-practicals will run on devices as small as a mobile 'phone.  However, the best experience is on a PC using a mouse which gives very precise control, but if you are limited to a small device, consider using a stylus or a blue tooth mouse.

 

The gamma ray source can be moved by placing the mouse cursor on it and using the scroll wheel (or dragging if using onscreen controls).

You can move the lead block between the ruler and the source by putting the mouse cursor over the block and using the mouse scroll wheel (or dragging if using onscreen controls). This will cut off the gamma rays moving in the direction of the detector and will enable you to get a good reading for the background radiation count. You may need to move the source to the right to enable the movement of the lead shield.

This shows the lead block moved in position to block the radiation from the source.

You can drop down to the level of the table by using the page down key (or the eye down icon when using onscreen controls), and you can zoom in and out on the apparatus using the plus and minus keys (or the magnifier icons when using the onscreen controls). You will find this useful when accurately placing the source on the ruler.

A closeup that shows how the position of the source can be read from the ruler by using the pointer built into the source carrier.

Notice the pointer in the source carrier in the above screen shot that enables you to accurately position the source when used with the zoom feature.

The Results

Create a table that has columns for the time period, the total count, the count rate, the corrected count rate (taking account of the background radiation), the distance, and 1 over the root of the count rate.

InverseSquareGraph.jpg

When you have found all the values, plot the graph of the last two columns, which should be a straight line.

Further Discussion

Why does your straight line not go through the origin?

Do we know the exact positions of the source and the detector?

Can we use the graph to tell us the relative positions of the source and the detector?

This section is adapted from material developed by Dr Robert Lucas and is related to the book High School and Undergraduate Physics Practicals, published by CRC Press.

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