Big Bang Nucleosynthesis

Reaction network · primordial element abundances · baryon density dependence
Baryon density Ω_b h² η ≈ 6.1×10⁻¹⁰
Neutron lifetime (s) 879 s
Neff (relativistic species) 3.0
Big Bang Nucleosynthesis (BBN) occurred during the first ~20 minutes of the universe, when temperatures fell from ~10¹² K to ~10⁹ K. A network of nuclear reactions converted free neutrons and protons into light nuclei: D, ³He, ⁴He, ⁷Li. The ⁴He mass fraction Y_p ≈ 0.245 is primarily set by the n/p ratio at freeze-out, controlled by the neutron lifetime and Neff. The D/H ratio is a sensitive baryometer — higher η destroys more deuterium via p+D→³He. Observations agree with ΛCDM (η ≈ 6.1×10⁻¹⁰) to ~1%.