Physics · IGCSE 0625 · §5.1–5.2

Nuclear Physics

Almost all of an atom is empty space — but its tiny, dense nucleus holds the mass, the charge, and the restless energy we call radioactivity.

Physics · 0625 Topic 5 of 6

The nuclear atom

nucleus (protons + neutrons) orbiting electrons
FIG 5.1 The nuclear atom: a dense central nucleus of protons and neutrons, with electrons in orbit far beyond it.

An atom is almost entirely empty space. Its mass and positive charge are crammed into a central nucleus thousands of times smaller than the atom itself, with electrons in orbit far beyond.

Nucleus and electrons

An atom has a small, positively charged nucleus surrounded by negatively charged electrons in orbit. A neutral atom has equal numbers of protons and electrons. An atom becomes a positive ion if it loses electrons, or a negative ion if it gains them.

Definition
Ion
A charged atom: positive if it loses electrons, negative if it gains them. Only electrons are gained or lost — the nucleus is unchanged.

ExtendedThe scattering experiment

Firing alpha particles at a thin metal foil provides the evidence for the nuclear model. Most pass straight through — so the atom is mostly empty space. A few are deflected, and a very few bounce back — so the nucleus is tiny, holds most of the mass, and is positively charged (it repels the positive alpha particles).

α particles gold foil
FIG 5.2 Most alpha particles pass through; a rare one rebounds from the nucleus.
Examiner note
Only electrons are gained or lost in forming ions. The nucleus is unchanged.
Why this matters
In the scattering experiment most alpha particles passed straight through the foil; a few bounced back — proof of a tiny, dense, positive nucleus.

The nucleus, nuclides and isotopes

The nucleus is built from two particles — protons and neutrons. How many of each there are fixes which element it is, and which version, or isotope, of that element.

Definition
Proton and nucleon number
Proton number Z: the number of protons; it defines the element. Nucleon number A: the total of protons and neutrons, so neutrons = A − Z.
Definition
Isotope
Atoms of the same element — the same Z — with a different number of neutrons. Carbon-12 and carbon-14 both have 6 protons but 6 and 8 neutrons.

Protons, neutrons and notation

The nucleus contains positively charged protons and uncharged neutrons. Their relative charges are +1, 0 and −1 for proton, neutron and electron. In nuclide notation the nucleon number A is written above and the proton number Z below the element symbol. The proton number Z sets the element; the nucleon number A is the total of protons and neutrons; so the number of neutrons is A − Z.

A Z X nucleon number proton number
FIG 5.3 Nuclide notation: nucleon number above, proton number below the element symbol.

Isotopes are atoms of the same element — the same Z — with different numbers of neutrons. For example, carbon-12 and carbon-14 both have 6 protons but 6 and 8 neutrons.

Examiner note
Relative charges are exactly +1 (proton), 0 (neutron) and −1 (electron) — learn these.

Fission and fusion

This whole section is Extended — Papers 2 and 4 only. Two opposite nuclear processes release enormous energy: splitting a heavy nucleus apart, and joining light nuclei together. Both are described qualitatively — the syllabus asks for the idea and a balanced nuclide equation, not energy values.

Definition
Fission and fusion
Fission — the splitting of a large, unstable nucleus into two smaller nuclei, releasing energy. Fusion — the joining of two light nuclei to form a heavier nucleus, releasing energy.

ExtendedFission: splitting nuclei

Nuclear fission is the splitting of a large, unstable nucleus into two smaller nuclei, usually triggered when it absorbs a neutron. Extra neutrons and energy are released; the mass of the products is fractionally less than the original, the lost mass appearing as energy. This is the process used in nuclear power stations.

ExtendedFusion: joining nuclei

Nuclear fusion is the joining of two light nuclei to form a heavier one, again with a tiny loss of mass released as energy. It needs extremely high temperature and pressure, which is why it powers stars but is so hard to reproduce on Earth.

Examiner note
Balance the equation: nucleon numbers (top) and proton numbers (bottom) must each add up to the same on both sides. Fission and fusion mass–energy changes are described qualitatively, without numerical values.
Why this matters
Fusion of hydrogen into helium is the energy source of the Sun and every star.

Detecting radioactivity

A low level of radiation is around us at all times. Before measuring any source, this background must be accounted for — otherwise every reading is too high.

Background radiation

Background radiation comes from natural sources: radon gas in the air, rocks and buildings, food and drink, and cosmic rays from space. Radon gas is typically the largest single source. Ionising radiation is measured with a detector (such as a Geiger-Müller tube) connected to a counter, giving a count rate in counts per second or per minute.

Definition
Background radiation
The low-level ionising radiation always present in the environment — from radon gas, rocks and buildings, food and drink, and cosmic rays from space.
relative contribution to background radon gas rocks & buildings cosmic rays
FIG 5.4 Radon gas is typically the largest single source of background radiation.
Examiner note
Count rate is measured in counts/s or counts/minute — not in becquerels, at this level. Extended: corrected count rate = measured count rate − background count rate.

Alpha, beta and gamma radiation

An unstable nucleus emits radiation spontaneously and in a random direction. There are three kinds — alpha, beta and gamma — and they differ sharply in what they are, how strongly they ionise, and how far they penetrate.

Definition
The three types
α — a helium nucleus, relative charge +2. β — a fast electron, relative charge −1. γ — a high-frequency electromagnetic wave, no charge.

Nature, ionising and penetrating power

Alpha is the most ionising but least penetrating — stopped by a sheet of paper or skin. Beta is moderately ionising and penetrating — stopped by a few millimetres of aluminium. Gamma is the least ionising but most penetrating — only reduced by thick lead or concrete.

α β γ paper aluminium lead
FIG 5.5 Penetrating power: alpha stops at paper, beta at aluminium, gamma only weakens through lead.

ExtendedDeflection and ionising effect

In an electric or magnetic field, alpha (+) and beta (−) are deflected in opposite directions, with beta deflected more because it is much lighter; gamma is undeflected. Alpha is the most ionising because it has the greatest charge and kinetic energy, so it interacts most strongly with the atoms it passes.

Examiner note
The most ionising radiation is the least penetrating: alpha ionises most but is stopped by paper. In a field, alpha and beta deflect in opposite directions; gamma is undeflected.

Radioactive decay

When an unstable nucleus emits radiation, it changes. Alpha and beta decay leave behind the nucleus of a different element entirely — a transformation written down as a balanced decay equation.

Definition
Decay is spontaneous and random
After alpha or beta decay, the nucleus becomes a different element. Alpha decay: A falls by 4, Z by 2. Beta decay: A is unchanged, Z rises by 1. Gamma emission changes neither.

A change of element

Radioactive decay is a spontaneous, random change in an unstable nucleus that emits alpha or beta particles and/or gamma radiation. After alpha or beta decay the nucleus becomes a different element.

In alpha decay the nucleus loses 2 protons and 2 neutrons, so A falls by 4 and Z by 2. In beta decay a neutron becomes a proton plus an electron (the beta particle), so A is unchanged and Z rises by 1. Gamma emission changes neither.

Worked example: radium-226 (Z = 88) emits an alpha particle. Alpha decay removes 4 nucleons, so A = 226 − 4 = 222, and 2 protons, so Z = 88 − 2 = 86 (radon).

Examiner note
Alpha decay: A falls by 4, Z by 2. Beta decay: A is unchanged, Z rises by 1. Balance both A and Z on each side of the equation.

Half-life

Decay is random, so we cannot say when a single nucleus will decay. But across a large sample the pattern is utterly reliable: in each half-life, half of what remains decays away.

Definition
Half-life
The time taken for half the nuclei of an isotope in a sample to decay. After one half-life half remain, after two a quarter, after three an eighth.

Halving, and halving again

The half-life is the time for half the nuclei in a sample to decay. After one half-life half remain, after two a quarter, after three an eighth, and so on — a steadily falling decay curve.

count rate time 1 half-life 2
FIG 5.6 A decay curve: the count rate halves over each successive half-life.

Worked example: a source’s count rate falls from 800 to 100 counts/s and its half-life is 5 hours. The halvings 800 → 400 → 200 → 100 are 3 half-lives, so the time taken is 3 × 5 = 15 hours.

Examiner note
Count half-lives by repeated halving: each halving of the count rate is one half-life. In Extended work, subtract the background count rate first.

Uses of radioactivity and safety

Ionising radiation damages living cells — it can cause cell death, mutations and cancer. Its uses, and the way it is handled safely, both come down to matching and controlling the radiation.

Definition
Matching radiation to the task
Each use is chosen by matching the type of radiation and the half-life to the job: penetrating power decides which radiation reaches where it is needed; half-life decides how long the source stays useful and safe.

ExtendedCommon uses

Smoke alarms use an alpha source to ionise the air, so smoke disrupts the current and triggers the alarm. Sterilising equipment and irradiating food to kill bacteria use gamma, which penetrates sealed packaging. Thickness control of paper or metal uses beta, whose transmission through the sheet changes with its thickness. Diagnosis and treatment of cancer use gamma, directed to image or destroy affected tissue.

Dangers and handling

Ionising nuclear radiation harms living things — it can cause cell death, mutations and cancer. Radioactive materials are therefore moved with tongs or handling tools, used at arm’s length, and stored in lead-lined containers well away from people.

Safety precautions for all ionising radiation reduce the dose received by: minimising the time of exposure, maximising the distance between the source and living tissue, and placing shielding (such as lead or concrete) to absorb the radiation.

Examiner note
Justify a use by naming the radiation and the reason, e.g. gamma for sterilising because it penetrates packaging. Three safety precautions earn the marks: reduce exposure time, increase distance, and use shielding.
Why this matters
A smoke alarm in the ceiling contains a tiny alpha source quietly ionising the air.

Exam advice

Common mistakes

Confusing ionising and penetrating
Alpha is the most ionising but the least penetrating. The two properties run opposite to each other.
Wrong decay changes
Alpha decay lowers A by 4 and Z by 2; beta decay leaves A unchanged and raises Z by 1.
Ignoring background radiation
In Extended half-life work, subtract the background count rate before reading off half-lives.
Predicting a single nucleus
Decay is random — you cannot say when one nucleus decays, only the average for a large sample.
Putting values on fission energy
Fission and fusion mass–energy changes are described qualitatively, without numerical values.

Model answer

A source’s count rate falls from 640 to 80 counts/s in 18 hours. (a) Find the half-life. (b) Predict the count rate 6 hours later.
[4 marks]
Mark 1
Count the halvings
640 → 320 → 160 → 80 is 3 half-lives.
Mark 2
Find the half-life
Half-life = 18 ÷ 3 = 6 hours.
Mark 3
Relate the extra time to the half-life
A further 6 hours is one more half-life.
Mark 4
Halve the count rate again
80 → 40 counts/s.

Recall checklist

  • Describe the nuclear atom and the alpha-scattering evidence for it.
  • Define proton number, nucleon number and isotope, and read nuclide notation.
  • Describe nuclear fission and fusion qualitatively and balance a nuclide equation (Extended).
  • Name the sources of background radiation and correct a count rate for it (Extended).
  • Compare alpha, beta and gamma for nature, ionising power and penetrating power.
  • State the changes to A and Z in alpha and beta decay and write balanced decay equations.
  • Define half-life and use it in calculations.
  • Justify the uses of radioactivity by radiation type and half-life (Extended).
  • State the dangers of ionising radiation and the three safety precautions.

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