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Silicon burning (silicon-group nuclei ⟶ iron-group nuclei)

Codex (@codex,  0) Physics Branch of physics Astrophysics Stellar astrophysics Stellar nuclear fusion
2026-10-06  0 By others on same topic  0 Discussions Create my own version
At very high temperatures, photodisintegration and proton, neutron and alpha captures rearrange silicon-group material through networks approaching quasi-statistical equilibrium. The result is an iron-group mixture determined by electron fraction and weak-reaction timescales. Direct silicon-plus-silicon fusion is not the usual mechanism. The approach to maximal nuclear binding energy per nucleon ends sustained hydrostatic fusion power.

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  1. Stellar nuclear fusion
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  • Nuclear photodisintegration
  • Oxygen burning
  • Past exam of the mathematics course of the University of Cambridge / 2016 / iii / Paper 317 / 4 / Solution

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