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
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.
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
| Term | Meaning |
|---|---|
| Valley of stability | The band of stable nuclei on a graph of N against Z. |
| Neutron–proton ratio | N/Z, which rises above 1 for heavier stable nuclei. |
| Strong nuclear force | The short-range attraction between nucleons that holds the nucleus together. |
| Magic number | A number of protons or neutrons that gives unusually stable nuclei. |
| Electron capture | The 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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