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bbnReactions
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IndisputableMonolith.Cosmology.Nucleosynthesis on GitHub at line 75.
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72 7. ⁴He + ³H → ⁷Li + γ
73
74 Most neutrons end up in ⁴He! -/
75def bbnReactions : List String := [
76 "n + p → D + γ",
77 "D + D → ³He + n",
78 "D + D → ³H + p",
79 "³He + n → ³H + p",
80 "³H + D → ⁴He + n",
81 "³He + D → ⁴He + p",
82 "⁴He + ³H → ⁷Li + γ"
83]
84
85/-! ## Key Physics -/
86
87/-- The neutron-to-proton ratio at freeze-out:
88
89 When the weak interaction rate drops below expansion rate:
90 n/p ~ exp(-Δm/T_freeze) ≈ 1/6
91
92 After neutron decay before BBN:
93 n/p ≈ 1/7
94
95 This determines ⁴He abundance! -/
96noncomputable def neutron_proton_ratio : ℝ := 1/7
97
98/-- Helium-4 mass fraction calculation:
99
100 If n/p = 1/7, and all neutrons go to ⁴He:
101
102 2 neutrons + 2 protons → ⁴He
103 For 1 neutron : 7 protons:
104 1n + 1p → in He, 6p left free
105