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Theme E — Nuclear and Quantum Physics

E.3.11 Nuclear Stability — IB Physics HL Revision Notes & Topical Questions

5 min read 9 parts Lesson 28 of 45 1 quiz

📚 IB Physics HL Hub / Topical Revision
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Curriculum Equation Key قوانين الرقم الهيدروجيني والاتزان الأيوني - pH & Acid-Base Equilibrium FormulasFast Exam Solution
pH = -log[H⁺] | pOH = -log[OH⁻] | pH + pOH = 14 | [H⁺][OH⁻] = 10⁻¹⁴
Word Equation & Conditions: الرقم الهيدروجيني = -لوغاريتم تركيز أيون الهيدروجين | pH + pOH = 14
Location & Specifications: الاتزان الأيوني، كيمياء 3 ثانوي، التحصيلي، و AP Chemistry.
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Lesson summary

E.3.11 Nuclear Stability — IB PHYSICS HL notes: Use the N–Z graph, the strong force and the neutron–proton ratio to explain nuclear stability and predict decay modes.Common elements — most have N and Z below 20, plus iron with Z = 26 and N = 30Reason — lighter nuclei with fewer p…

  • Light nuclei
  • Heavy nuclei
  • Electromagnetic repulsion
  • Extra neutrons
  • Above the band (too many neutrons)
  • Below the band (too many protons)

Part 1 of 7Stable nuclei

Common elements
  • Common elements most have N and Z below 20, plus iron with Z = 26 and N = 30
Reason
  • Reason lighter nuclei with fewer protons are much more stable than heavy ones
N–Z graph
  • N–Z graph plotting N against Z shows a band of stable nuclei called the valley of stability
Light nuclei
  • Light nuclei for Z below about 20 the stable nuclei follow N = Z
Heavy nuclei
  • Heavy nuclei the band bends upward because stable nuclei need N greater than Z
Ratio
  • N/Z rises from 1 to about 1.5 for lead
Limit
  • Limit no nuclide above Z = 83 is stable

Part 2 of 7Why nuclei become unstable

Too many neutrons
Too many protons
Too many nucleons, so the nucleus is too heavy
Too much energy
Goal
  • Goal an unstable nucleus decays to become more stable

Part 3 of 7Strong force and neutron–proton ratio

1Strong force
  • Strong force at 1–3 fm nucleons are bound
  • Below about 1 fm it is repulsive and prevents collapse
2Electromagnetic repulsion
  • Electromagnetic repulsion it acts between protons at longer range, so more protons mean more instability
3Extra neutrons
  • Extra neutrons they space the protons apart to cut repulsion and add strong-force binding
4Why
  • Why electrostatic repulsion grows roughly as Z2 while the strong force reaches only nearest neighbours

Part 4 of 7Predicting the decay mode

Predicting the decay mode
Above the band (too many neutrons)
  • β− decay turns a neutron into a proton
  • N falls by 1 and Z rises by 1
Below the band (too many protons)
  • β+ decay or electron capture turns a proton into a neutron
  • N rises by 1 and Z falls by 1
Large nuclei (A above about 200)
  • α decay removes 2 protons and 2 neutrons
  • N and Z each fall by 2
Excited nucleus
  • Excited nucleus gamma emission, with N and Z unchanged
N/Z
  • N/Z a nuclide with N/Z too high for its Z is a β− emitter and one with N/Z too low is a β+ emitter or electron capturer

Part 5 of 7Decay chains on the N–Z grid

α decay
  • α decay two squares down and two left
β− decay
  • β− decay one square down and one right
β+ decay
  • β+ decay one square up and one left
Uranium-238 series
  • Uranium-238 series each alpha step changes A by 4 so the members have A = 238 − 4n
  • It ends at lead-206 after eight alpha and six beta decays
Energy
  • Energy a nuclide is unstable if some decay leads to a lower total mass

Part 6 of 7Magic numbers and pairing

Magic numbers
  • Magic numbers nuclei with 2, 8, 20, 28, 50, 82 or 126 protons or neutrons are unusually stable
Shell model
  • Shell model nucleons occupy discrete energy levels with filled shells giving extra stability
Pairing
  • Pairing nuclei with even numbers of both protons and neutrons are more stable

Part 7 of 7More from the specification

More from the specification
Nuclear stability band
  • Nuclear stability band plotting neutron number versus atomic proton number provides an empirical means to predict radioactive alpha or beta decay.
Activity of a Radioactive Sample
  • Activity A is the rate of decay of a radioactive source, measured in becquerels (Bq),
    • (A = -dN / dt = λN)
  • where 1 Bq corresponds to one nuclear disintegration per second.
Mathematics of Half-Life Determination
  • Half-life can be determined graphically from a plot of activity or nucleus count against time, identifying the time interval required for the measured quantity to fall to 50% of its initial value.
Radioactive Dating Applications
  • By comparing the current activity of carbon-14 or uranium isotopes in an ancient sample to initial levels, geologists and archaeologists determine ages spanning thousands to billions of years using N = N₀ * e^(-λt).
Background Radiation and Correction
  • Background radiation originating from cosmic rays, radon gas,
  • and natural minerals must be measured and subtracted from raw detector counts to obtain accurate sample activity.
Alpha particle
  • Helium nucleus, charge +2.
Background radiation
  • Radiation that is always present in the environment.
Decay equation
  • An equation in nuclide notation with balanced nucleon and proton numbers.
Ionising radiation
  • Radiation with enough energy to remove electrons from atoms
Penetrating power
  • How far radiation travels through a material.
Radiation
  • Transfer by electromagnetic waves, requiring no medium
Radioactive
  • Describes a nucleus that decays spontaneously and randomly.
Activity
  • Number of decays per second of a sample.
Half-life
  • Time for half the nuclei of an isotope to decay.
Constant
  • Not changing.
Isotope
  • Atom of the same element with a different number of neutrons.
Isotopes
  • Nuclei with the same proton number but different neutron numbers.
Source
  • Reservoir at TH providing heat QH

Key terms

TermMeaning
Valley of stabilityThe band of stable nuclei on a graph of N against Z.
Neutron–proton ratioN/Z, which rises above 1 for heavier stable nuclei.
Strong nuclear forceThe short-range attraction between nucleons that holds the nucleus together.
Magic numberA number of protons or neutrons that gives unusually stable nuclei.
Electron captureThe capture of an orbital electron by a proton, forming a neutron and a neutrino.

Avoid these mistakes

1
Reversing the sides of the band — too many neutrons gives β− decay.
2
Believing N = Z for all stable nuclei — heavier nuclei need N greater than Z.
3
Thinking alpha decay changes N/Z dramatically — it removes equal numbers of both.
4
Forgetting that no nuclide above Z = 83 is stable.
5
Assuming more neutrons is always more stable.

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