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
| Property | Alpha | Beta-Minus | Gamma |
|---|---|---|---|
| Nature | Helium nucleus | Electron | Electromagnetic wave |
| Charge | +2 | -1 | 0 |
| Relative Mass | Large | Very small | Zero rest mass |
| Speed | Moderate | High | |
| Ionising Power | High | Medium | Low |
| Penetrating Power | Low | Medium | High |
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:
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