Worked examples — Fusion — D-T reaction, solar fusion (p-p chain), tokamak - ICF
The scenario matrix
Every fusion/nuclear-energy problem lives in one of these cells. The examples below are labelled by the cell they cover, so together they leave no gap.
| Cell | Case class | What's tricky about it | Example |
|---|---|---|---|
| A | , two products (fusion) | standard mass-defect arithmetic | Ex 1 |
| B | Energy split between two products | momentum conservation, not equal split | Ex 2 |
| C | (endothermic / "uphill") | negative answer means needs energy | Ex 3 |
| D | (degenerate, at the B/A peak) | fusing near iron gives ~nothing | Ex 4 |
| E | Multi-step chain, net | intermediate species cancel; neutrinos leak | Ex 5 |
| F | Coulomb barrier (limiting energy scale) | why we need millions of kelvin | Ex 6 |
| G | Real-world word problem | reactor power ↔ reaction rate | Ex 7 |
| H | Exam twist: given, not masses | back out from binding energies | Ex 8 |
Conversion we will reuse constantly:
Cell A — Standard exothermic fusion ()
Forecast: two hydrogens fusing move uphill on the B/A curve → energy out → I expect a small positive number, a few MeV (smaller than D–T's 17.6, because we're not making the super-stable He).
- Sum the reactants. . Why this step? By the master formula, depends only on total mass before vs after — reactants first.
- Sum the products. . Why this step? Same rule, the "after" side.
- Mass defect. . Why this step? The mass that vanished is what becomes energy — this is $E=mc^2$ in action.
- Convert. . Why this step? Turn the missing mass into MeV using the ↔MeV bridge.
Verify: ✓ (fusion should release energy), and MeV MeV ✓ (D–D is a weaker step than D–T, matching the forecast). Units: ✓.
Cell B — How the energy splits between products
When a reaction starts with the reactants essentially at rest, the two products fly apart back-to-back with equal and opposite momentum. They do not share energy equally — the lighter one is faster and carries more kinetic energy.
The figure below draws exactly this picture: the reaction point at rest, a long cyan arrow for the light, fast neutron flying one way, and a short amber arrow for the heavy, slow He recoiling the other way. Equal-length momentum, unequal kinetic energy — look at how much longer the cyan velocity arrow is.

Forecast: neutron is ~3× lighter, so it should grab ~3× the energy — roughly three-quarters of the total.
- Set the ratio. . Why this step? Inverse-mass rule from the box above.
- Total the parts. shares of MeV → each share MeV. Why this step? Divide the pie into equal slices, then hand them out.
- Assign. MeV; MeV. Why this step? Give 3 slices to the lighter (faster) neutron, 1 to the heavier He.
Verify: MeV = total ✓. Neutron got the larger share ✓. Same logic gives D–T's famous split (a ratio, since the — the He nucleus — is 4× the neutron mass) — reassuring consistency.
Cell C — Endothermic reaction ()
Forecast: Be is famously unstable — it falls apart almost instantly. That hints the product is not more bound, so I expect (nature won't hand out free energy here).
- Sum reactants. . Why this step? Two alpha particles (He nuclei) combining — total their mass.
- Product mass. . Why this step? The single product's mass is the "after" side.
- Mass defect. . Why this step? Negative! Mass went up, so energy was absorbed, not released.
- Convert. . Why this step? Same bridge; the sign carries through.
Verify: ✓, matching that Be is unbound relative to two alphas (it lives ~ s). This is exactly why stars need the triple-alpha trick — a third helium must arrive during that fleeting instant. See Stellar Nucleosynthesis. Units ✓.
Cell D — Degenerate case: fusion at the peak ()
Forecast: both sit near the peak (~8.5–8.8 MeV/nucleon), so the gain per nucleon is tiny; total should be a mere few MeV — vanishing compared to D–T, and essentially "worthless" as fuel.
- Binding of reactants. MeV. Why this step? Total binding for each nucleus. More binding = more stable.
- Binding of product. MeV. Why this step? Same, for the single heavy product.
- = gain in binding. MeV. Why this step? Energy released = how much more tightly bound the product is (binding released as KE).
Verify: is positive but tiny per nucleon: MeV/nucleon vs D–T's MeV/nucleon — about 18× less useful. And just past Fe/Ni the peak flattens and turns over, so the next step would give then negative. This is the "degenerate" cell: at the very peak, fusion yields essentially nothing. See Nuclear Fission — beyond the peak, it's splitting that pays.
Cell E — Multi-step chain, net (with leaking neutrinos)
Forecast: the parent note quotes ~26.7 MeV; I expect the mass-defect route to land there, with a couple percent then vanishing as neutrinos escape.
- Reactant mass. . Why this step? Four hydrogen atoms in, total their atomic mass.
- Product mass. . Why this step? Using atomic helium mass already includes 2 electrons, cancelling the 2 positrons' annihilation — a neat bookkeeping shortcut.
- Mass defect. . Why this step? This total missing mass is the entire chain's energy budget.
- Convert. . Why this step? Bridge to MeV.
- Subtract the leak. Neutrinos carry off ~2% (~0.5 MeV); usable sunlight ≈ MeV. Why this step? Neutrinos barely interact — that energy leaves the Sun instantly, never becoming heat.
Verify: MeV matches Worked Example 2 of the parent ✓. The slow first step (a proton must -decay mid-collision, a rare weak-interaction event) is why the Sun burns for ~10 billion years. Units ✓.
Cell F — The Coulomb barrier (limiting energy scale)
The figure below plots potential energy versus separation : a cyan wall rising as the nuclei approach (Coulomb repulsion), then a sudden drop into a deep amber well once they touch at nuclear range (the strong force). The white dot marks the barrier top — the ~288 keV summit a nucleus must climb (or tunnel through) before it can fall into the well and fuse.

Forecast: the parent said "hundreds of keV." I expect a few hundred keV.
- Write the barrier. . Why this step? Electrostatic potential energy of two point charges at separation — the wall's peak.
- Plug numbers (SI, joules). . Why this step? Do it in SI to avoid unit traps, convert at the end.
- Convert to keV. . Why this step? J; report in nuclear units.
Verify: keV — squarely in the "hundreds of keV" range the parent claimed ✓. A gas at temperature has typical thermal energy (with the Boltzmann constant J/K); to reach keV energies you'd naively need K, yet reactors run at "only" K. The gap is bridged by the high-energy tail plus quantum tunnelling through the wall. Units ✓.
Cell G — Real-world word problem (power ↔ reaction rate)
Forecast: MeV is a minuscule joule amount, so we'll need a colossal rate — but the fuel mass will be tiny because nuclei are so light. That's fusion's headline: little fuel, huge power.
- Energy per reaction in joules. J. Why this step? Power is in J/s, so convert the per-reaction energy to J.
- Reactions per second. . Why this step? Power = (energy per event) × (events per second) ⇒ divide.
- Deuterons per day. One D per reaction: deuterons/day. Why this step? Multiply the per-second rate by seconds in a day ().
- Mass of deuterium. kg. Why this step? Number of atoms × mass per atom = total mass.
Verify: kg of deuterium per day for a gigawatt — about 100 grams, roughly the mass of an apple, powering a city ✓. This is the "little fuel, huge power" punchline, and it's why confinement research is worth billions. Units: J ÷ (J/reaction) = reactions ✓.
Cell H — Exam twist: from values, not masses
Forecast: should reproduce ~17.6 MeV — that's the consistency check the examiner is fishing for.
- Reactant binding. MeV; MeV; total MeV. Why this step? ; sum both reactant nuclei.
- Product binding. MeV; the free neutron has ; total MeV. Why this step? Same rule; the loose neutron adds nothing (nothing binds it).
- = gain in binding. . Why this step? Energy released equals how much more bound the products are — that binding surplus emerges as kinetic energy of the and neutron.
Verify: MeV matches the mass-defect MeV ✓ — two independent routes to the same number, the hallmark that you understand why works, not just the formula. Units: MeV throughout ✓.
Recall Self-test the whole matrix
Which cell has , and what does that physically mean? ::: Cell C — the products are less bound (e.g. Be from two alphas); the reaction absorbs energy instead of releasing it. In an at-rest reaction, which product carries more kinetic energy? ::: The lighter one — energy splits inversely to mass, since and . Two ways to compute ? ::: (1) mass defect ; (2) (binding of products) − (binding of reactants). They must agree. Why must we heat plasma to K even though ? ::: The ~288 keV Coulomb barrier repels the nuclei; only the tail particles + tunnelling make it through.