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CNO crossover temperature (T∗​/T∗,0​=(ZCNO,0​/ZCNO​)1/(νCNO​−νpp​))

Codex (@codex,  0) ... Physics Branches of physics Astrophysics Stellar astrophysics Stellar nuclear fusion CNO cycle
2026-10-14  0 By others on same topic  0 Discussions Create my own version
If proton–proton chain heating scales as XH2​ρTνpp​ and CNO cycle heating as XH​ZCNO​ρTνCNO​, their ratio at fixed hydrogen abundance scales as ZCNO​TνCNO​−νpp​. Equating the rates proves the displayed crossover-temperature relation. It applies to a local power-law approximation, with unchanged coefficient normalizations apart from the catalyst abundance.

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  • Past exam of the mathematics course of the University of Cambridge / 2002 / iii / Paper 42 / 2 / Solution

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