Radioactive decay and half-life - CCEA

Part of Physics (Single Science)Unit 1: Atomic and nuclear physics

What are the key points about radioactive decay and half-life?

  • To understand why some are .

  • What is , and radiation - and what are the differences between them?

  • To understand nuclear decay equations.

  • How to measure the activity of radioactive sources.

  • How to calculate .

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What is radioactivity?

Stable and unstable nuclei

Radioactivity is caused by the nucleus of an being unstable.

The of and in a determines whether a nucleus will be stable or unstable.

Too many neutrons or protons can upset this balance making the nucleus unstable.

Carbon-12 is stable and has six protons and six neutrons.

However as the number of protons increases, more neutrons are needed to keep the nucleus stable.

For example lead, lead-206 has 82 protons and has 124 neutrons.

Nuclei with too many, or too few, neutrons do exist naturally but are unstable and will disintegrate (or decay) by emitting radiation.

This is called radioactive decay.

It is important to realise that radioactive nuclei disintegrate:

  • spontaneously

  • and randomly.

Spontaneously means that the process of radioactive decay can not be speeded up or slowed down by physical factors, e.g. temperature or pressure etc.

Random means that we cannot predict when an individual unstable nucleus will decay.

Key facts

  • Some nuclei are unstable.

  • They disintegrate and emitting radiation.

  • Such nuclei are described as radioactive.

What is ionising radiation?

The radiation emitted from unstable nuclei is called ionising radiation because as it passes through it can dislodge outer from atoms causing them to become .

What are the different types of radioactive decay?

An unstable nucleus can decay by emitting an alpha particle, a beta particle, or a gamma ray.

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What is alpha radiation?

An unstable nucleus can emit a ‘package’ of two protons and two neutrons, called an alpha particle, to become more stable.

Alpha radiation is made up of a stream of alpha particles emitted from unstable nuclei within a radioactive substance.

An alpha particle is also a helium-4 nucleus.

It is written as

\(_{2}^{4}\textrm{He}\) and is also sometimes written as \(_{2}^{4}\alpha\).

Alpha decay causes the of the nucleus to decrease by four and the of the nucleus to decrease by two.

Image gallerySkip image gallerySlide 1 of 9, An unstable nucleus., 1. An unstable nucleus can decay by the emitting an alpha particle to become more stable.

What is the alpha decay equation?

\(_{Z}^{A}\textrm{X} \rightarrow _{Z-2}^{A-4}\textrm{Y} +\ _{2}^{4}\textrm{He}\) or \(_{2}^{4}\textrm{α}\)

Note that the mass numbers and atomic numbers are equal (i.e. they balance) on both sides of the equation.

Example

Alpha decay of Uranium-238

\(_{92}^{238}\textrm{U} \rightarrow _{90}^{234}\textrm{Th} +_{2}^{4}\textrm{He}\)

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What is beta radiation?

An unstable nucleus can emit a fast-moving electron called a beta (β) particle, to become more stable.

Beta radiation is made up of a stream of beta particles emitted from unstable nuclei within a radioactive substance.

Beta radiation is normally emitted from unstable nuclei in which the number of neutrons is much larger than the number of protons.

A beta particle has a that can be considered to be zero, so its mass number is zero, and as the beta particle is an electron, it can be written as: \(_{-1}^{~0}\textrm{e}\)

Sometimes, it is also written as: \(_{-1}^{~0}\beta\).

Image gallerySkip image gallerySlide 1 of 8, An unstable nucleus with too many neutrons., 1. An unstable nucleus that has too many neutrons can decay by the emitting a beta particle to become more stable.

Key fact

The beta particle is an electron but it has come from the nucleus, not the of the atom.

Electrons are not normally found in the nucleus but, in an unstable nucleus, a neutron can split into a positive proton and a negative electron.

The proton remains inside the nucleus, but the electron is ejected at high speed.

This is called beta decay.

Beta decay causes the of the nucleus to increase by one (because there is an extra proton) but the remains the same (because the total number of protons and neutrons remains unchanged).

What is the equation for beta decay?

\(_{Z}^{A}\textrm{X} \rightarrow _{Z+1}^{A}\textrm{Y} + _{-1}^{0}\textrm{e}\) or \(_{-1}^{~0}\beta\)

Example

Beta decay of carbon-14

\(_{6}^{14}\textrm{C} \rightarrow_{7}^{14}\textrm{N} +\ _{-1}^{0}\textrm{e}\)

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What is gamma radiation?

Gamma radiation does not consist of particles but as short wavelength, high energy electromagnetic radiation emitted from unstable nuclei.

It is normally emitted alongside or radiation.

Image gallerySkip image gallerySlide 1 of 4, A nucleus after emitting an alpha or beta particle., 1. After emitting an alpha or beta particle, the nucleus will often still be ‘excited’ and will need to lose energy.

Gamma ray emission causes no change in the number of particles in the nucleus meaning both the atomic number and mass number remain the same.

It can be written as γ or \(_{0}^{0}\textrm{γ}\)

What is the gamma decay equation?

\(_{X}^{A}\textrm{X}\rightarrow_{Z}^{A}\textrm{Y}+_{0}^{0}\textrm{γ}\) or γ

Example

Beta and gamma decay of cobalt-60

\(_{27}^{60}\textrm{Co}\rightarrow_{28}^{60}\textrm{Ni}+_{-1}^{0}\textrm{e}+_{0}^{0}\textrm{γ}\)

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What are the properties of nuclear radiations?

The different types of radiation are often compared in terms of their , their and how far they can travel in the air.

SymbolStopped byPenetration powerIonising powerRange in air
AlphaαSkin/paperLowHigh4-6 centimetre (cm)
Betaβ5 mm aluminiumMediumLow≈ 1 metre (m)
GammaγReduced by thick lead/concreteHighVery low> 1 kilometre (km)
The properties of different nuclear radiations by their penetrating power.

All types of radioactive decay can be detected by a , or G-M tube.

What are the key points about the different radiations?

Alpha radiation

  • Alpha particles are helium consisting of two and two emitted from unstable nuclei \(_{2}^{4}\textrm{α}\)

  • Alpha radiation is stopped by a few (4-6) centimetres of air or a thin sheet of paper.

  • Alpha decay: \(_{Z}^{A}\textrm{X}\rightarrow_{Z-2}^{A-4}\textrm{Y}+_{2}^{4}\textrm{He}\) or \(_{2}^{4}\textrm{α}\)

  • The of the new nucleus decreases by 4.

  • The of the new nucleus decreases by 2.

  • Alpha particles are relatively heavy and so produce the most .

Beta radiation

  • Beta particles are fast moving emitted from an unstable nucleus.

  • Beta radiation is stopped by several metres of air or a thin (~5 mm) sheet of aluminium \(_{-1}^{~0}\beta\).

  • Beta decay: \(_{X}^{A}\textrm{X}\rightarrow_{Z+1}^{A}\textrm{Y}+_{-1}^{0}\textrm{e}\) or \(_{-1}^{~0}\beta\)).

  • The mass number of the new nucleus stays the same.

  • The atomic number of the new nucleus increases by 1.

  • Beta particles are much lighter than alpha particles and so produce a great deal less ionisation.

Gamma radiation

  • Gamma radiation is high energy electromagnetic waves emitted from unstable nuclei.

  • Gamma radiation easily passes through air, paper, skin and aluminium but can be partly blocked by thick lead or concrete.

  • Emission of gamma radiation leaves mass number and atomic number unchanged.

  • Gamma rays produce the least ionisation.

Question

Complete the following decay equation:

\(_{86}^{226}\textrm{Ra}\rightarrow_{Z}^{A}\textrm{Rn}+_{2}^{4}\textrm{He}\)

Question

Polonium-210 decays to lead-206. Polonium (Po) has atomic number 84 and lead (Pb) has atomic number 82.

Which type of decay occurs?

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How to measure amounts of radiation?

The activity of a radioactive source is the number of decays per second from the unstable present in the source.

The simplest unit of activity is the Becquerel (Bq).

A source that emits one particle per second has an activity of one Bq.

Activity can also be measured in counts per minute.

Since is a process, it is always good practice to determine the average count rate rather than to measure the counts that occur in just one second or one minute.

Radioactivity can be detected using a Geiger-Muller tube connected to a counter.

When alpha particles, beta particles or gamma rays enter the GM tube the counter clicks and the count is displayed on the screen.

The number of counts per second or per minute is called the count rate.

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What is background radiation?

A will detect radiation even when there is no apparent radioactive source present.

This is because radioactive material is found naturally all around us.

Key Fact

Background radiation is the radiation detected when there are no known radioactive sources present.

Examples of natural sources of background radiation:

  • Radioactive rocks in the ground.

  • Cosmic rays from space.

How to measure the background radiation

  • Remove all known sources of radioactivity from the room.
  • Set the counter to zero.
  • Switch on and start a stop clock.
  • After 20 minutes switch off. Record the count.
  • Divide the count by 20 to calculate the count rate per minute.

The background count rate is measured over a period of 20 minutes because of the random nature of radioactive decay.

Dividing by 20 enables the average count rate per minute to be determined.

Background count rate is typically 18 counts per minute which does not present a serious health risk to humans.

Key fact

The background count rate must be subtracted from any other count rate when measuring the activity of a radioactive source. This is known as the corrected count rate.

Corrected count rate = Measured count rate – Background count rate

Question

A scientist measures the background radiation level in their lab and records the following results:

Experiment numberCounts in 20 mins
1367
2354
3359

Calculate the average reading for the background radiation level in counts per minute.

Question

The scientist then measures the activity of a sample of strontium-90 in the same lab.

The average reading is 309 counts per minute.

Calculate the corrected activity of the sample of strontium-90.

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What is half-life?

is a and process.

A block of radioactive material will contain many trillions of nuclei and not all nuclei are likely to decay at the same time.

As the process of radioactive decay is random, it is impossible to tell when a particular nucleus will decay but given that there are so many of them, it is possible to say that a certain number will decay in a certain time.

This is called the half-life.

Key fact

Half-life is the time taken for the activity of the source to fall to half its original value.

The illustration below shows how a radioactive sample is decaying over time.

How a radioactive sample decays over time.

From the start of timing it takes two days for the count to halve from 80 Bq down to 40 Bq.

It takes another two days for the count rate to halve again, this time from 40 Bq to 20 Bq.

The half-life of this source is 2 days.

Note that this second two days does not see the count drop to zero, only that it halves again.

A third, two-day period from four days to six days sees the count rate halving again from 20 Bq down to 10 Bq.

This process continues and although the count rate might get very small, it does not drop to zero completely.

The half-life of radioactive carbon-14 is 5,730 years.

If a sample of a tree (for example) contains 64 grams (g) of radioactive carbon after 5,730 years it will contain 32 g, after another 5,730 years that will have halved again to 16 g.

How to set out half-life calculations

Example 1 – If the half-life is known

Image gallerySkip image gallerySlide 1 of 5, Becquerels of a substance whose half-life is known - at 0 seconds., 1. The activity of a radioactive source was found to be 1200 Bq. The half-life is 6 hours (t½ = 6 hours). What will the activity be after 24 hours? Start by writing out what you know initially, (at t = 0)...

Example 2 – If the half-life is not known

Image gallerySkip image gallerySlide 1 of 6, At t = 0, activity is at 3600 Bq., 1. The activity of a radioactive source was found to be 3600 Bq. After one hour it had fallen to 450 Bq. Calculate the half-life of the source. Start by writing out what you know initially, (at t = 0). Then state what you would know after one half-life.

How to calculate how much of an isotope remains

It should also be possible to state how much of a sample remains or what the activity or count should become after a given length of time.

This could be stated as a fraction, decimal or .

For example the amount of a sample remaining after four half-lives could be expressed as:

  • a fraction - a \(\frac{\text{1}}{\text{2}}\) of a \(\frac{\text{1}}{\text{2}}\) of a \(\frac{\text{1}}{\text{2}}\) of a \(\frac{\text{1}}{\text{2}}\) remains which is \(\frac{\text{1}}{\text{2}}\) x \(\frac{\text{1}}{\text{2}}\) x \(\frac{\text{1}}{\text{2}}\) x \(\frac{\text{1}}{\text{2}}\) = \(\frac{\text{1}}{\text{16}}\) of the original sample.

  • a decimal - \(\frac{\text{1}}{\text{16}}\) = 0.0625 of the original sample

This could then be incorporated into other data.

So, if the half-life is two days, four half-lives is 8 days.

Question

If a sample with a half-life of 2 days has a count rate of 3,200 Bq at the start, what is its count rate after 8 days?

Question

The half-life of cobalt-60 is 5 years. If there are 100 g of cobalt-60 in a sample, how much will be left after 15 years?

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How much do you know about radioactive decay and half-life?

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