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Radioactive decay and half-life - CCEAStable and unstable nuclei

Radioactivity was first noticed by French physicist, Henri Becquerel, in 1896, when he observed that some photographic plates which had been stored close to a uranium compound had become partly exposed or ‘fogged’.

Part of Physics (Single Science)Atomic and nuclear physics

Stable and unstable nuclei

The balance 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.

Elements with fewer protons, such as the ones near the top of the periodic table, are stable if they have the same number of neutrons and protons.

For example carbon, 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.

Graph showing the rate of decay with he number of protons against the number of neutrons. Purple line on the graph shows the stability line and the green line is N=Z.

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.

This means that the process of radioactive decay can not be speeded up or slowed down by artificial means (spontaneous decay).

It also means that we cannot tell when a particular unstable nucleus will decay (random decay).

Key points

  • Some nuclei are unstable.
  • They disintegrate, emitting radiation randomly, and spontaneously.
  • Such nuclei are described as radioactive.

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