Topic 6

Nuclear Physics

Natural radioactivity, half-life, nuclear reactions (fission & fusion), and radiation hazards.

A. Natural Radioactivity

What is Radioactivity?

Radioactivity is the spontaneous emission of radiation from an unstable nucleus. Discovered by Henri Becquerel (1896). Pioneered by Marie Curie.

α Alpha
⁴₂He
Charge: +2 Mass: 4 amu
Ionisation: Highest
Penetration: Lowest

Stopped by a sheet of paper. Dangerous if inhaled/ingested.

β Beta
e⁻ or e⁺
Charge: ±1 Mass: ~0
Ionisation: Medium
Penetration: Medium

Stopped by aluminium sheet. Can penetrate skin.

γ Gamma
γ (photon)
Charge: 0 Mass: 0
Ionisation: Lowest
Penetration: Highest

Needs thick lead or concrete. Most dangerous externally.

RadiationSymbolChargeMassPenetrationIonisation
Alpha (α)⁴₂He+2 (2p, 2n)4 amuLowest (stopped by paper)Highest
Beta (β)e⁻ or e⁺−1 or +1~0Medium (stopped by aluminium)Medium
Gamma (γ)γ00Highest (needs lead/concrete)Lowest
Alpha (α)
Symbol⁴₂He
Charge+2 (2p, 2n)
Mass4 amu
PenetrationLowest (stopped by paper)
IonisationHighest
Beta (β)
Symbole⁻ or e⁺
Charge−1 or +1
Mass~0
PenetrationMedium (stopped by aluminium)
IonisationMedium
Gamma (γ)
Symbolγ
Charge0
Mass0
PenetrationHighest (needs lead/concrete)
IonisationLowest

B. Half-Life

Half-Life Formula & Decay Table

Time for half the radioactive nuclei in a sample to decay

Radioactive Decay N = N₀ × (½)ⁿ N₀ = initial number · n = number of half-lives elapsed · n = t / t½
0
100%
1
50%
2
25%
3
12.5%
4
6.25%

C. Nuclear Reactions

Nuclear Fission

  • A heavy nucleus splits into two smaller nuclei + neutrons + energy
  • Example: ²³⁵U + n → Ba + Kr + 3n + energy
  • Used in nuclear power plants and atomic bombs
  • Chain reaction: neutrons released cause further fissions

Nuclear Fusion

  • Two light nuclei combine to form a heavier nucleus + energy
  • Example: 2 Hydrogen (deuterium) nuclei → Helium + energy
  • Powers the Sun and other stars
  • Releases MORE energy than fission — future energy source
⚡ MCQ Tip Alpha = stopped by paper, highest ionisation. Beta = stopped by aluminium. Gamma = needs lead, lowest ionisation. Half-life: after each half-life, quantity halves. Fission = splitting. Fusion = joining.

D. Radiation Hazards & Safety

Hazards, Effects & Safety Measures

HazardEffectSafety Measure
Ionising radiationDamages DNA, causes cancer and mutationsLead shielding, distance, minimise exposure time
Alpha particlesDangerous if inhaled or ingestedAvoid inhalation; not a skin hazard externally
Beta particlesCan penetrate skin; damages tissuesAluminium shielding; protective clothing
Gamma raysDeep tissue penetration; most dangerous externallyThick lead or concrete walls
Nuclear wasteLong-term radioactive contaminationDeep geological storage; sealed containers

Live Animation: Alpha Decay & Half-Life

Radioactive Decay — Alpha Particle Emission

Watch nuclei spontaneously emit alpha particles. Half-life counter updates in real time.

Remaining nuclei: 40 Decayed: 0 Elapsed time: 0.0 s Half-lives passed: 0 % remaining: 100%
8
40

Quick MCQ Revision

Formula / FactMeaning
N = N₀ × (½)ⁿRadioactive decay — n = number of half-lives
n = t / t½Number of half-lives = total time ÷ half-life
Alpha (α)⁴₂He · charge +2 · stopped by paper · highest ionisation
Beta (β)e⁻ · charge ±1 · stopped by aluminium · medium ionisation
Gamma (γ)EM wave · no charge/mass · needs lead · lowest ionisation
FissionHeavy nucleus SPLITS → energy + neutrons (nuclear power)
FusionLight nuclei JOIN → energy (powers the Sun)
Half-lifeAfter 1 half-life → 50% remains. After 2 → 25%. After 3 → 12.5%
BecquerelDiscovered radioactivity (1896)
Key