Nuclear physics
The atom and nucleus, alpha, beta and gamma radiation, half-life calculations, decay equations, fission and fusion, and radiation safety.
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In 30 seconds
- An atom has a tiny, dense, positive nucleus (protons + neutrons) with electrons in shells around it.
- Isotopes have the same number of protons but different numbers of neutrons.
- Alpha (stopped by paper) ionises most. Beta (stopped by aluminium). Gamma (reduced by thick lead) is the most penetrating.
- Decay is random and spontaneous. Half-life is the time for half the nuclei to decay.
- EXT Decay and fission/fusion equations must balance both the top (A) and bottom (Z) numbers.
By the end you can
- Describe the structure of the atom and use nuclide notation.
- Tell alpha, beta and gamma apart by their nature, ionisation and penetration.
- Use half-life with tables and graphs and correct for background radiation. EXT
- Write balanced decay equations. EXT
- Describe fission and fusion, and explain the uses and dangers of radiation.
1The atom
Inside the atom
| Particle | Relative charge | Relative mass | Where |
|---|---|---|---|
| proton | +1 | 1 | nucleus |
| neutron | 0 | 1 | nucleus |
| electron | −1 | about 1/1836 | in shells around the nucleus |
- A neutral atom has equal numbers of protons and electrons.
- An atom that loses electrons becomes a positive ion. An atom that gains electrons becomes a negative ion.
Evidence for the nucleusEXTENDED
- Most α particles went straight through, so most of an atom is empty space.
- A few were deflected, so the centre of the atom is positive and repels the positive α particles.
- Very few bounced straight back, so the positive nucleus is tiny, dense and has most of the mass.
Nuclide notation and isotopes
Proton number (Z) — the number of protons in the nucleus. It decides the element. EXT It is also the charge of the nucleus.
Nucleon number (A) — the number of protons plus neutrons. EXT It decides the mass of the nucleus.
Isotopes — atoms of the same element (same Z) with different numbers of neutrons (different A).
How many protons, neutrons and electrons are in a neutral atom of 146C? How does it differ from 126C?
- protons = Z = 6
- neutrons = A − Z = 14 − 6 = 8
- electrons = 6 (neutral atom)
- 126C has 6 neutrons, so the two are isotopes with different numbers of neutrons
2Radioactivity
Background radiation
Background radiation — ionising radiation that is always around us.
- Natural sources: radon gas (from rocks), rocks and buildings, food and drink, and cosmic rays from space.
- It is detected with a Geiger–Müller tube connected to a counter. The reading is a count rate in counts per second or counts per minute.
- EXT Corrected count rate = measured count rate − background count rate.
EXT A source gives 156 counts per minute. The background is 12 counts per minute. Find the corrected count rate.
- corrected = 156 − 12 = 144 counts per minute
Alpha, beta and gamma
Radioactive decay — the spontaneous and random change of an unstable nucleus, giving out radiation. Spontaneous means nothing outside causes it (not heat, not pressure). Random means you cannot tell when one particular nucleus will decay, or in which direction the radiation goes.
| Alpha (α) | Beta (β) | Gamma (γ) | |
|---|---|---|---|
| what it is | 2 protons + 2 neutrons (a helium nucleus) | a fast electron from the nucleus | an electromagnetic wave |
| charge | +2 | −1 | 0 |
| ionising power | strongest | medium | weakest |
| stopped by | paper, a few cm of air | a few mm of aluminium | only reduced by thick lead or concrete |
| range in air | a few cm | about 1 m | very long |
- Ionisation means knocking electrons off atoms to make ions. This can damage living cells.
- EXT Alpha particles are big and heavily charged, so they ionise strongly and lose their energy over a very short distance.
Radioactive decay
- Alpha and beta decay change the nucleus into a different element. Gamma emission does not change the element — it just takes away spare energy.
- EXT Nuclei are unstable if they have too many neutrons or are too heavy. Emitting radiation makes the nucleus more stable.
- EXT In beta decay a neutron changes into a proton and an electron: n → p + e. The electron is emitted.
EXT Complete: 21084Po → ?82Pb + 42He
- Top numbers: 210 = ? + 4, so ? = 206
- Bottom numbers: 84 = 82 + 2 ✓
- 21084Po → 20682Pb + 42He
Half-life
Half-life — the time taken for half the nuclei of a radioactive isotope in a sample to decay. It is also the time for the count rate (activity) to fall to half.
A sample has a half-life of 6 hours and a count rate of 800 counts per minute. What is the count rate after 18 hours?
- 18 ÷ 6 = 3 half-lives
- 800 → 400 → 200 → 100 counts per minute
EXT A count rate is measured as 640, 320, 160 and 80 counts per minute at 0, 10, 20 and 30 minutes. Find the half-life.
- The count rate halves every 10 minutes
- half-life = 10 minutes
Uses of radiationEXTENDED
| Use | Radiation | Why |
|---|---|---|
| smoke alarm | alpha | alpha ionises the air so a small current flows; smoke absorbs it and the current falls; alpha cannot leave the alarm; long half-life |
| thickness of paper or foil | beta | more of the beta is absorbed by thicker sheet, so the count falls |
| sterilising food and surgical tools | gamma | passes through packaging and kills bacteria |
| medical tracer | gamma | passes out of the body to be detected; a short half-life means it soon disappears |
| treating cancer | gamma | penetrates the body and kills cancer cells |
Safety
- Ionising radiation causes cell death, mutations and cancer.
- Handle sources with tongs. Store them in lead-lined boxes, keep them away from people and label them with the hazard symbol.
- EXT Reduce exposure by: limiting time near the source, increasing distance (radiation spreads out), and using shielding (lead or concrete).
3Fission and fusion EXT
Nuclear fission
- In a nuclear power station the chain reaction is controlled. The energy heats water to make steam for a turbine.
Nuclear fusion
- Fusion powers the Sun and other stars. Researchers are working to use it for electricity, but it needs extreme temperatures to push positive nuclei close enough to join.
| Fission | Fusion | |
|---|---|---|
| what happens | a large nucleus splits | small nuclei join |
| example | uranium-235 | hydrogen isotopes |
| conditions | needs a neutron | needs about 10 million °C and a huge pressure |
| where | nuclear power stations | the Sun and stars |
4Test yourself
Test yourself — cover the answers first
Quick check
- State the relative charges of a proton, a neutron and an electron.
- How many neutrons are in 146C?
- Which radiation is most penetrating?
- Name two sources of background radiation.
- A source has a half-life of 12 days. What fraction is left after 36 days?
- What is an isotope?
Exam-style
- EXT A source gives a measured 340 counts per minute. The background is 40 counts per minute and the half-life is 2.0 hours. Find the measured count rate after 4.0 hours.
- Explain why a smoke alarm uses an alpha source. [3]
- EXT Describe and explain what the alpha-scattering experiment showed about the atom. [4]
- EXT Write the decay equation for 9038Sr emitting a beta particle. The new element is yttrium (Y).
- Explain why gamma rays, not alpha, are used as a medical tracer. [2]
Show answers
- +1, 0, −1
- 14 − 6 = 8
- gamma
- radon gas, rocks, food and drink, cosmic rays (any two)
- 36 ÷ 12 = 3 half-lives, (½)³ = 1/8
- An atom of the same element with a different number of neutrons.
- corrected = 340 − 40 = 300
4.0 h = 2 half-lives: 300 → 150 → 75
measured = 75 + 40 = 115 counts per minute - Alpha ionises the air, so a small current flows
smoke absorbs the alpha particles, so the current drops and the alarm sounds
alpha cannot escape from the alarm, so it is safe - Most α went straight through, so the atom is mostly empty space
a few were deflected through large angles, so the nucleus is positive
very few bounced back, so the nucleus is small and dense
the nucleus has most of the mass - 9038Sr → 9039Y + 0−1e
- Gamma passes out of the body so it can be detected
alpha would be stopped inside the body and do more damage to cells
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