Stellar NucleosynthesisProton-Proton Chain · Gamow Peak · Energy Generation

Stellar Parameters

Gamow Peak (keV)
ε (erg/g/s)
PP-I fraction
H lifetime (Gyr)
¹H+¹H²D+e⁺+ν
²D+¹H³He+γ
▶ PP-I: ³He+³He→⁴He+2¹H
▶ PP-II: ³He+⁴He→⁷Be→⁷Li→⁴He
▶ PP-III: ⁷Be+¹H→⁸B→⁸Be→2⁴He
Gamow window: balance between Maxwell-Boltzmann tail and tunneling probability. Peak at E₀ = (πe²μc²/2)^(2/3)·(kT)^(2/3).
Energy gen: ε ∝ ρX²T^n where n≈4 for pp-chain. Branch ratios depend strongly on T.