Fission
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What is the 'mass defect' of a nucleus?
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All Flashcards in Topic 5.4
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5.4.115 cards
What is the 'mass defect' of a nucleus?
(Mass of the separate protons + neutrons) − (mass of the bound nucleus). The nucleus is the **lighter** one.
What is the 'binding energy' of a nucleus?
The energy equivalent of the mass defect (E = mc²) — the energy needed to **pull the nucleus apart** into separate nucleons.
What is 'binding energy per nucleon'?
Binding energy ÷ number of nucleons (A). It lets you **compare the stability** of different nuclei fairly.
Which equation links the mass defect to the binding energy?
$E = mc^{2}$ — mass-energy equivalence (given in the data booklet). Here m is the mass defect.
Fast way to convert a mass defect in u into energy in MeV?
Multiply Δm (in u) by **931.5**, because 1 u = 931.5 MeV c⁻².
On the binding-energy-per-nucleon curve, what does 'higher' mean?
**More tightly bound = more stable.** The curve peaks near iron (A ≈ 56), the most stable nuclei.
Why does fusion of light nuclei release energy?
It moves **up** the steep left side of the curve — the product is more tightly bound — so energy is released.
Why does fission of heavy nuclei release energy?
It moves **up** the gentle right side of the curve toward iron — the products are more tightly bound — so energy is released.
Which nucleus sits at the peak of the curve?
Iron (around **A ≈ 56**) — the most tightly bound, most stable nucleus.
Fusion vs fission — which releases more energy per unit mass of fuel?
**Fusion** — it climbs the steep light-nuclei side, giving several times more MeV per nucleon than fission.
A nucleus has Δm = 0.030 u and 4 nucleons. Binding energy per nucleon?
E = 0.030 × 931.5 ≈ 28 MeV total, then 28 ÷ 4 ≈ **7 MeV per nucleon**.
What is the strong nuclear force?
An **attractive**, **short-range** (≈ 1–3 fm) force between nucleons that holds the nucleus together against the protons' electric repulsion.
Why does the strong force not pull nucleons into one point?
Below about 0.5 fm it becomes strongly **repulsive**.
How do you turn a mass given in MeV c⁻² into an energy?
Drop the c⁻²: a mass defect of 2.0 MeV c⁻² is a binding energy of **2.0 MeV**.
Why is the binding energy per nucleon roughly constant above A ≈ 60?
The strong force is **short-range**: each nucleon is bound only by its nearest neighbours, however big the nucleus.
5.4.214 cards
What is nuclear fission?
A **large nucleus splits** into two smaller nuclei, releasing **energy** and a few spare **neutrons**.
What is induced fission?
Fission **triggered** by a nucleus **absorbing a neutron**, which makes it unstable so it splits (not happening on its own).
What is a chain reaction?
Each fission releases neutrons that go on to cause **more** fissions — one fission triggers the next.
What does 'self-sustaining' mean for a chain reaction?
The chain **keeps itself going** without any extra neutrons being added from outside.
How many neutrons does one fission typically release?
About **2 or 3** (plus two daughter nuclei and a lot of energy).
Condition for a STEADY (critical) chain reaction?
On average **exactly one** neutron per fission goes on to cause the **next** fission.
If N neutrons are released per fission, how many are lost or absorbed when steady?
**N − 1.** One continues the chain; the rest must be lost or absorbed.
What happens if fewer than N − 1 neutrons are lost per fission?
More than one continues, so the rate **grows** — the reaction is **supercritical**.
What happens if more than N − 1 neutrons are lost per fission?
Fewer than one continues, so the reaction **dies out** — it is **subcritical**.
Why does each fission release energy?
The products are slightly **lighter** than the original — that tiny **mass defect** becomes energy via **E = mc²**.
Subcritical, critical, supercritical — what do they mean?
Subcritical = dying out; **critical = steady**; supercritical = growing. Set by how many neutrons continue per fission.
What is spontaneous fission?
A heavy nucleus splitting **on its own**, without absorbing a neutron; like induced fission it releases energy.
How do you find the energy released in a fission reaction from masses?
Δm = (mass of U + neutron) − (fragments + all neutrons out); E = Δm × 931.5 MeV.
About how much energy does one U-235 fission release?
About **200 MeV** (3.2 × 10⁻¹¹ J).
5.4.315 cards
What are the four key components of a nuclear reactor?
**Fuel**, **moderator**, **control rods** and **heat exchanger**.
What is the function of the moderator?
It **slows down the fast neutrons** so they are more likely to cause the next fission.
What is the function of the control rods?
They **absorb spare neutrons** to keep the chain reaction steady (or shut it down).
What is the function of the fuel?
It is the material (e.g. **uranium-235**) that **undergoes fission** and releases the energy.
What is the function of the heat exchanger?
It **carries heat out of the core** to boil water into steam, which drives a turbine.
Name two suitable moderator materials.
**Water** or **graphite** (both slow neutrons effectively).
Name two suitable control-rod materials.
**Boron** or **cadmium** (both strongly absorb neutrons).
Why must the neutrons be slowed down?
A **slow** neutron is **much more likely** to be absorbed by U-235 and cause fission than a fast one — so slowing them keeps the chain reaction going.
What happens when the control rods are lowered (inserted)?
More neutrons are **absorbed**, so the chain reaction **slows down**. Raising them speeds it up.
Moderator vs control rods — what is the difference?
Both act on neutrons: the moderator **slows** them (helps fission); the control rods **absorb** them (limit fission).
How does the reactor turn nuclear energy into electricity?
Fission heats the core → the heat exchanger makes **steam** → steam spins a **turbine** → the turbine drives a **generator**.
Given data-booklet formula for the energy released by a fission?
$E = mc^{2}$ — the lost mass (mass defect) times the speed of light squared.
What is the function of the shielding in a nuclear reactor?
Thick **steel and concrete** round the core **absorb neutrons and gamma rays**, protecting people outside.
Why are the products of fission radioactive?
They have **too many neutrons** to be stable, so they decay (mostly beta and gamma); some for thousands of years.
How is high-level nuclear waste stored?
Cooled in water ponds, then sealed in **glass and steel** and buried **deep underground** in stable rock for thousands of years.
Topic 5.4 study notes
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