Know that a β-particle is a high-speed electron emitted from the nucleus, formed when a neutron changes into a proton and an electron and a reduction in the number of excess neutrons; the following change in the nucleus occurs during β-emission neutr
5.2.3 Radioactive Decay – β‑Particle Emission
What is β‑decay?
Spontaneous, random nuclear transformation that changes one element into another.
One of the three decay modes required by the Cambridge IGCSE syllabus (α, β, γ).
In β‑decay a neutron in the nucleus is converted into a proton, a high‑speed electron (the β‑particle) and an antineutrino.
The nuclear reaction
The fundamental change can be written as
\$n \;\rightarrow\; p^{+} + e^{-} + \bar{\nu}_e\$
where n = neutron, p⁺ = proton, e⁻ = β‑particle, \(\bar{\nu}_e\) = antineutrino (carries away excess energy and momentum).
After decay: Z = 20, A = 39 (calcium). The element changes, but the mass number does not.
Summary of nuclear changes
Property
Before β‑decay
After β‑decay
Neutron count
n
n − 1
Proton count
p
p + 1
Atomic number (Z)
Original Z
Original Z + 1
Mass number (A)
Original A
Unchanged (A)
Comparison of the three types of radiation
Radiation
Particle / quantum
Charge
ΔZ
ΔA
Ionising power
Penetrating ability
Typical shielding
α‑particle
Helium nucleus (42He)
+2
–2
–4
High
Low
Paper (≈0.5 mm) or a few cm of air
β‑particle
Electron (e⁻)
–1
+1
0
Medium
Medium
Aluminium (≈2–3 mm) or Plexiglas
γ‑ray
High‑energy photon
0
0
0
Low
High
Lead (≈2 cm) or several centimetres of concrete
Detection of β‑particles
β‑particles are recorded as electrical pulses in a Geiger‑Müller tube, scintillation counter or semiconductor detector.
The instrument shows a count‑rate (counts s⁻¹). To obtain the net rate, subtract the background count‑rate measured with no source present (see 5.2.1).
Because β‑particles are charged, they ionise air; the ionisation current is the basis of most detection methods.
Half‑life – definition and simple calculation
Half‑life (T½): the time required for half of a given number of radioactive nuclei to decay.
For IGCSE the decay law can be written as
\$N = N0\left(\frac{1}{2}\right)^{t/T{½}}\$
where N₀ is the initial number of nuclei, N the number remaining after time t.
Example: 9038Sr has T½ = 28.8 years. After 57.6 years (2 × T½) the activity is \(\frac{1}{4}\) of the original.
Safety precautions for β‑radiation
β‑particles are stopped by a few millimetres of aluminium or Plexiglas; use these as shields when handling sources.
Wear gloves and use forceps or tongs to avoid direct skin contact.
Store sources in lead containers (lead also stops any accompanying γ‑radiation) and keep them out of the laboratory when not in use.
Apply the three‑principle rule: minimise time, maximise distance, and use appropriate shielding.
Common β‑emitters and their applications
146C – carbon dating (archaeology, geology).
3215P – medical tracer in blood‑pool studies.
9038Sr – industrial gauges and thickness monitors.
3H (tritium) – self‑luminous exit signs and nuclear‑fusion research.
40K – natural background radiation; used in geological dating.
Key points to remember
β‑decay converts a neutron into a proton, an electron (β‑particle) and an antineutrino.
Atomic number increases by 1; mass number remains unchanged.
β‑particles have medium penetrating power; a few mm of aluminium stops them.
The decay is spontaneous and random; the half‑life characterises the rate of decay.
Detection is usually by a Geiger‑Müller tube, scintillation counter or semiconductor detector; always subtract background.
Safety: shield with aluminium, keep sources away from skin, minimise exposure time, and store in lead containers.
Suggested diagram: a neutron inside a nucleus transforms into a proton while emitting an electron (β‑particle) and an antineutrino.
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