Deuterium bottleneck

Light nuclei cannot accumulate until cooling makes deuterium sufficiently resistant to photodissociation, delaying nucleosynthesis after weak freeze-out.

Table of contents 121 3
- Deuterium equilibrium abundance Deuterium bottleneck 91 1
  - Baryon-density effect on primordial helium Deuterium equilibrium abundance 40
- Free-neutron decay after freeze-out Deuterium bottleneck 13

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Big Bang nucleosynthesis
Cosmology
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