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Nuclear Physics

5. Nuclear Physics — Cambridge IGCSE Physics 0625 Revision Notes & Topical Questions

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Curriculum Equation Key Radioactive Decay & Half-Life FormulasFast Exam Solution
N(t) = N₀ × (1/2)t / t½ | λ = ln(2) / t½ ≈ 0.693 / t½ | E = Δm × c²
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Lesson summary

Nuclear Physics — notes: Describe the nuclear atom, fission and fusion, background radiation, the properties of alpha, beta and gamma radiation, decay equations and half-life.Nuclear model — a small, dense, positive nucleus is surrounded by orbiting negative electrons.Size — an …

  • Neutral atom
  • Experiment
  • Observations
  • Conclusions
  • Positive ion
  • Negative ion

Part 1 of 22Structure of the atom

Structure of the atom
Nuclear model
  • Nuclear model a small, dense, positive nucleus is surrounded by orbiting negative electrons.
Size
  • Size an atom has a radius of about 1 x 10-10 m;
    • the nucleus is over 10 000 times smaller but holds almost all of the mass.
Terms
  • Terms the atom is nucleus plus electrons; the nucleus is protons plus neutrons.
Neutral atom
  • Neutral atom has equal numbers of protons and electrons.

Part 2 of 22Rutherford alpha scattering (Extended)

Experiment
  • Experiment in 1909 Geiger and Marsden, directed by Rutherford, fired alpha particles (He2+) at thin gold foil to test the plum pudding model.
Observations
  • Observations most alpha particles passed straight through, some were deflected, and a few bounced back.
Conclusions
  • Conclusions the atom is mostly empty space, the nucleus is positive and repels alpha particles (deflection),
    • and it is tiny and contains most of the mass (a few rebound).
    • (most pass through)
Impact
  • Impact the plum pudding model could not explain rebounds, so the nuclear model replaced it.

Part 3 of 22Atoms and ions

Ion
  • Ion a charged atom or group of atoms formed by gaining or losing electrons.
Positive ion
  • Positive ion forms when electrons are lost, leaving more protons than electrons.
Negative ion
  • Negative ion forms when electrons are gained, leaving more electrons than protons.
Net charge
  • Net charge the overall charge; 5 protons, 5 neutrons and 6 electrons give a net negative charge.

Part 4 of 22Proton number, nucleon number and nuclide notation

Proton (atomic) number Z
  • Proton (atomic) number Z is the number of protons;
    • it fixes the element and equals the number of electrons in a neutral atom.
  • Hydrogen Z = 1, sodium Z = 11, uranium Z = 92.
Nucleon (mass) number A
  • Nucleon (mass) number A is the number of protons plus neutrons; neutrons = A - Z.
  • Sodium 23: 23 - 11 = 12 neutrons.
Electron mass
  • Electron mass is negligible, so electrons are not counted in A.
Nuclide notation
  • Nuclide notation is AZX with A on top and Z at the bottom;
    • a nuclide is a group of atoms with the same protons and neutrons.
Example
  • 19779Au has 79 protons, 118 neutrons and 79 electrons.

Part 5 of 22Isotopes

Isotopes
  • Isotopes are atoms of the same element with the same number of protons but different numbers of neutrons.
Hydrogen
  • Hydrogen hydrogen-1 (0 neutrons), deuterium hydrogen-2 (1 neutron) and tritium hydrogen-3 (2 neutrons);
    • about 2 in 10 000 hydrogen atoms are deuterium and tritium is far rarer.
Stability
  • Stability isotopes with an imbalance of protons and neutrons tend to be unstable and decay.
Identifying isotopes
  • Identifying isotopes same element symbol and proton number but different nucleon number, for example uranium-238 and uranium-235 or carbon-12 and carbon-14.

Part 6 of 22Relative charge and mass

ParticleRelative chargeRelative mass
Proton+11
Neutron01
Electron-1negligible (about 1/2000)
Fundamental charge
  • 1.6 x 10-19 C, the size of the charge on a proton or electron.
Nuclear charge
  • = number of protons x +1; chromium-52 with 24 protons has charge +24.
Nuclear mass
  • = number of nucleons x 1;
    • chromium-52 has relative mass 52 and one relative mass unit is about 1.67 x 10-27 kg.

Part 7 of 22Nuclear fission

1Definition
  • Definition the splitting of a large unstable nucleus into two smaller nuclei.
2Process
  • Process a neutron strikes an unstable nucleus, which splits into two daughter nuclei, two or three neutrons and gamma rays.
3Equation
  • 23592U + 10n → 9236Kr + 14156Ba + 3 10n + energy.
  • Nucleon numbers
    • 235 + 1 = 92 + 141 + 3;
      • proton numbers: 92 + 0 = 36 + 56 + 0.
4Energy
  • Energy nuclear energy becomes kinetic energy of the fast-moving products;
    • the products have slightly less mass, the missing mass having become energy.
5Fuels
  • Fuels large nuclei such as uranium and plutonium are used in nuclear power stations.

Part 8 of 22Nuclear fusion

Definition
  • Definition two light nuclei join to form a heavier nucleus.
Stars
  • Stars fuse hydrogen nuclei into helium, releasing huge energy.
Conditions
  • Conditions extremely high temperature and pressure are needed, so fusion is hard to reproduce on Earth.
Equation
  • 21H + 11H → 32He + energy.
Energy and mass
  • Energy and mass the product has slightly less mass than the reactants;
    • 1 kg of hydrogen fusing releases as much energy as burning about 10 million kg of coal.
Balancing example
  • 235U + 1n → 96Rb + 137Cs + N1n: 236 = 233 + N so N = 3.

Part 9 of 22Background radiation

Definition
  • Definition radiation present around us all the time; the count rate varies from place to place.
Natural sources
  • Natural sources radon gas, rocks and buildings, food and drink (for example potassium-40 in bananas), cosmic rays and carbon-14 in biological material.
    • (alpha emitter from uranium decay in rocks)
Man-made sources
  • Man-made sources medical X-rays, CT scans, tracers and radiotherapy;
    • nuclear waste;
    • fallout from weapons tests;
    • and accidents such as Chernobyl.
Largest contributions
  • Largest contributions radon gas, food and drink, and cosmic rays.
Radon
  • Radon is colourless, tasteless and odourless and is dangerous mainly if inhaled in large quantities.

Part 10 of 22Detecting radiation and count rate

Count rate
  • Count rate is the number of detected decays per second or minute;
    • it falls with distance because radiation spreads out.
Geiger-Muller tube
  • Geiger-Muller tube each absorbed particle gives an electrical pulse to a counter which clicks and shows the count rate.
Other detectors
  • Other detectors photographic film in badges, ionisation chambers, scintillation counters and spark counters.
Example
  • 16 000 decays in 1 hour is 16 000 / 3600 = 4.5 per second.
Naming
  • Naming say Geiger-Muller tube (GM counter), not just radiation detector.

Part 11 of 22Correcting for background radiation

Method
  • Method measure the count with no source and subtract it from readings with the source.
Data example
  • Data example counts per minute at 0.2, 0.4, 0.6, 0.8, 1.0, 1.2, 1.4 m were 180, 67, 29, 17, 15, 15, 15.
  • Beyond 1 m the readings stay constant at 15 counts per minute, which is the background.

Part 12 of 22Random radioactive decay

Spontaneous and random
  • Spontaneous and random a nucleus decays without outside influence and in a random direction.
Implications
  • Implications every nucleus has equal probability of decaying, you cannot predict which or when,
    • and only the probability in a time period can be given.
  • The decay rate is unaffected by surrounding conditions.
Unstable nuclei
  • Unstable nuclei are unstable due to too many protons or neutrons or being very large.
    • (carbon-14 has two extra neutrons compared with stable carbon-12)
Becoming stable
  • Becoming stable they emit high-energy particles or waves, which carry energy away.

Part 13 of 22Alpha, beta and gamma radiation

RadiationNatureChargeRange in airPenetrationIonising
Alpha (α)Helium nucleus (2 protons + 2 neutrons)+2A few cmStopped by paperHigh
Beta (β-)Fast electron from a neutron changing into a proton-1A few tens of cmStopped by a few mm of aluminium or PerspexModerate
Gamma (γ)Electromagnetic wave of highest energy0InfiniteReduced by thick leadLow
Trends
  • Trends range and penetrating power increase from alpha to gamma while ionisation decreases.
Identifying a source
  • Identifying a source count rate unchanged by paper but greatly reduced by 5 mm aluminium indicates beta.
    • (4320, 4218, 256, 34 example)

Part 14 of 22Ionisation

Ionisation
  • Ionisation occurs when radiation removes electrons from atoms, leaving positive ions.
Charge
  • Charge the larger the charge the more ionising: alpha (+2) most, beta (-1) moderate, gamma (0) least.
Kinetic energy
  • Kinetic energy alpha is heavy and most ionising;
    • beta is light but fast and moderately ionising;
    • gamma has no mass and is weakly ionising.

Part 15 of 22Deflection in fields (Extended)

Rule
  • Rule only charged, moving particles are deflected; gamma is never deflected.
Electric field
  • Electric field alpha moves towards the negative plate and beta towards the positive plate;
    • beta deflects more because it is lighter.
Magnetic field
  • Magnetic field alpha and beta deflect in opposite directions because their charges are opposite.

Part 16 of 22Nuclear stability and decay chains

Stable nuclei
  • Stable nuclei light nuclei have about equal numbers of protons and neutrons, while heavier nuclei need more neutrons to offset proton repulsion.
Hydrogen isotopes
  • H-1 is stable, H-2 is stable and H-3 is unstable.
    • (2 neutrons to 1 proton)
Heavy nuclei
  • Heavy nuclei such as uranium-238 are held together less strongly and decay in a chain by alpha and beta emission.
New element
  • New element after alpha or beta decay the daughter nucleus is a different element.
    • (parent Pu-239 to U-235 loses 2 protons and 2 neutrons)

Part 17 of 22Types of decay

DecayChange in nucleusMass numberAtomic number
AlphaEmits 2 protons and 2 neutronsDecreases by 4Decreases by 2
BetaA neutron becomes a proton and an electron is emittedUnchangedIncreases by 1
GammaEmits energy onlyUnchangedUnchanged
  • Beta-plus
    • a proton changing to a neutron exists but is not needed for this course.

Part 18 of 22Decay equations

Rule
  • Rule the sum of mass numbers and the sum of atomic numbers must be equal on both sides.
Alpha
  • AZX → A-4Z-2Y + 42α; for example 21284Po → 20882Pb + 42α.
Beta
  • AZX → AZ+1Y + 0-1β.
Gamma
  • AZX → AZX + 00γ.
Alpha example
  • 84 protons and 126 neutrons gives A = 210; alpha decay gives lead-206 with Z = 82.
Beta example
  • 11 protons and 13 neutrons gives A = 24; beta decay gives Z = 12 (magnesium-24).

Part 19 of 22Half-life

Definition
  • Definition the time taken for half of the nuclei of an isotope in a sample to decay.
    • (or for activity to halve)
Equal intervals
  • 100% to 50% takes the same time as 50% to 25%.
Using it
  • Using it after n half-lives the fraction left is (1/2)n;
    • read the half-life from a decay curve by finding the time for the count to halve, correcting for background first.
Example
  • Example a sample of 80 g with a half-life of 3 days has 20 g left after 6 days.

Part 20 of 22Uses of radioactivity

Uses of radioactivity
Smoke detectors
  • Smoke detectors americium-241 emits alpha particles that ionise air;
    • smoke reduces the current and sets off the alarm.
Thickness gauges
  • Thickness gauges beta radiation through paper or foil; the count rate falls as thickness increases.
Medical tracers and treatment
  • Medical tracers and treatment gamma emitters with short half-lives are used as tracers;
    • gamma sterilises equipment and treats cancer.
Dating
  • Dating carbon-14 half-life of 5700 years dates organic remains.
Choosing a source
  • Choosing a source consider type of radiation and a suitable half-life.

Part 21 of 22Dangers of radiation and safety

Harm
  • Harm ionising radiation damages cells and DNA, causing burns, mutations and cancer.
Alpha
  • Alpha is very harmful if inhaled or swallowed but is stopped by skin; gamma and beta penetrate the body.
Precautions
  • Precautions handle sources with tongs, store in lead-lined containers, keep distance and limit time of exposure, use shielding and wear dosimeter badges.
Dose
  • Dose the amount of radiation received by a person, which must be regulated.

Part 22 of 22Worked examples

  1. Gold is 19779Au. State the numbers of protons, neutrons and electrons. [1]1 mark

  2. A nucleus with 84 protons and 126 neutrons undergoes alpha decay. Find the daughter nucleus. [2]2 marks

  3. A Geiger counter records 16 000 decays in 1 hour. Calculate the count rate per second. [2]2 marks

  4. A source gives 4320, 4218, 256 and 34 counts with no material, paper, 5 mm aluminium and 5 mm lead. Identify the radiation. [2]2 marks

  5. Balance 235U + 1n → 96Rb + 137Cs + N1n. Find N. [2]2 marks

Key terms

TermMeaning
IsotopesAtoms of the same element with different numbers of neutrons.
Nuclear fissionSplitting of a large unstable nucleus into two smaller nuclei.
Nuclear fusionJoining of two light nuclei to form a heavier nucleus.
Background radiationRadiation present in the environment all the time.
Half-lifeTime for half the nuclei in a sample to decay.
IonisationRemoval of electrons from atoms by radiation.
Count rateNumber of decays detected per unit time.
Nucleon numberNumber of protons plus neutrons in a nucleus.

Avoid these mistakes

1
Saying the number of neutrons is the proton number — neutrons = nucleon number minus proton number.
2
Thinking beta particles come from outside the nucleus — a neutron changes into a proton and an electron.
3
Believing the decay of a particular nucleus can be predicted — decay is random and only probabilities can be given.
4
Forgetting to subtract background radiation before analysing source count rates.
5
Mixing up fission and fusion — fission splits a large nucleus; fusion joins light nuclei.

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