Radioactive Decay

Overview

Radioactive Decay is the spontaneous transformation of an unstable nucleus into a more stable nucleus, accompanied by the emission of radiation.

This topic links closely with:

Core Ideas

  • unstable nuclei may decay spontaneously into more stable nuclei
  • radioactive decay is random for individual nuclei but statistically predictable for large samples
  • alpha, beta-minus, and gamma emissions have different physical natures and different penetrating and ionising powers
  • nuclear equations must conserve nucleon number and charge
  • activity measures the rate of decay and is measured in becquerels

Unstable Nuclei

Some nuclei are unstable because of an unfavourable balance of:

  • protons and neutrons
  • strong nuclear force and electrostatic repulsion
  • excess nuclear energy

Such nuclei undergo radioactive decay to become more stable.

Examples include:

  • very heavy nuclei
  • nuclei with too many neutrons
  • nuclei in excited states

Spontaneous Nature of Decay

Radioactive decay is spontaneous.

This means:

  • no external trigger is needed
  • it occurs naturally
  • it cannot be stopped by ordinary physical or chemical means

It is generally unaffected by:

  • temperature
  • pressure
  • chemical state
  • electric fields
  • magnetic fields

Random Nature of Decay

Decay is also random.

This means:

  • it is impossible to predict when a particular nucleus will decay
  • each unstable nucleus has a constant probability of decay per unit time

However, for a large sample:

  • behaviour becomes predictable statistically
  • count rate and activity follow exponential decay

See Half-Life.

Activity Overview

Activity is the rate of nuclear decay.

Over a finite time interval, activity can also be viewed as the average number of decays per unit time.

SI unit:

Larger activity means more decays each second.

Alpha Decay

An alpha particle is:

It contains:

  • 2 protons
  • 2 neutrons

General form:

It occurs commonly in heavy nuclei.

Beta-Minus Decay

In beta-minus decay, a neutron changes into a proton and emits an electron.

General form:

Key changes:

  • nucleon number unchanged
  • proton number increases by 1

The antineutrino may be omitted depending on the syllabus treatment of nuclear equations.

Gamma Emission

Gamma radiation is electromagnetic radiation emitted by an excited nucleus.

Key changes:

  • no change in
  • no change in

Only the nuclear energy decreases.

Properties of Alpha, Beta and Gamma

PropertyAlphaBeta-MinusGamma
NatureHelium nucleusElectronElectromagnetic wave
Charge+2-10
Relative MassLargeVery smallZero rest mass
SpeedModerateHigh
Ionising PowerHighMediumLow
Penetrating PowerLowMediumHigh

Ionising Power vs Penetrating Power

Ionising Power

This is the ability to remove electrons from atoms.

Order:

Penetrating Power

This is the ability to pass through matter.

Order:

Typical shielding:

  • alpha: paper or skin
  • beta: aluminium sheet
  • gamma: thick lead or concrete

Behaviour in Electric and Magnetic Fields

Alpha

  • positively charged
  • deflected toward the negative plate
  • small deflection because of large mass

Beta-Minus

  • negatively charged
  • deflected toward the positive plate
  • larger deflection because of small mass

Gamma

  • no charge
  • not deflected

Field treatment is qualitative at H2 level.

Decay Equations Overview

Nuclear equations must conserve:

  • nucleon number
  • charge, equivalently proton number

Example alpha decay:

See Decay Equations and Conservation.

Conservation Laws Overview

In radioactive decay:

Conserved

  • total nucleon number
  • total charge
  • energy
  • momentum

Therefore

Nuclear equations must balance both the top and bottom numbers.

Safety Context

Radioactive emissions can ionise matter and damage living tissue.

Applications, hazards, and precautions are covered in:

Ionizing Radiation and Safety

Short Worked Examples

Example 1: Alpha Decay Daughter

After alpha emission:

Answer:

Example 2: Beta-Minus Decay Daughter

After beta-minus decay:

Answer:

Example 3: Gamma Emission

If excited cobalt emits gamma radiation:

  • the same element remains
  • the same remains
  • the same remains

Only the nucleus drops to a lower energy state.

Exam Relevance

Students should be able to:

  • distinguish spontaneous decay from random decay
  • compare alpha, beta-minus, and gamma radiation
  • describe ionising power, penetrating power, and field behaviour qualitatively
  • balance simple nuclear equations using conservation of nucleon number and charge
  • identify the correct daughter nucleus after a decay

Formula Sheet

Activity

Alpha Decay

Beta-Minus Decay

Gamma Emission

Common Exam Traps Overview

Students often confuse:

  • alpha with beta particles
  • ionising power with penetrating power
  • the wrong changes in and
  • gamma radiation with a charged massive particle
  • decay being caused by heating
  • random decay with unpredictable sample behaviour

See Radioactive Decay Common Exam Traps.

Quick Revision Summary

  • radioactive decay is spontaneous and random
  • unstable nuclei may emit alpha, beta-minus, or gamma radiation
  • alpha is massive, highly ionising, and weakly penetrating
  • beta has intermediate ionising and penetrating power
  • gamma is weakly ionising and strongly penetrating
  • nuclear equations conserve nucleon number and charge
  • large samples decay predictably even though individual nuclei decay randomly