Precision big bang nucleosynthesis with improved Helium-4 predictions
Cyril Pitrou, Alain Coc, Jean-Philippe Uzan, Elisabeth Vangioni

TL;DR
This paper refines the prediction of primordial helium-4 abundance by incorporating comprehensive corrections to weak interaction rates, achieving high-precision results consistent with recent observational improvements.
Contribution
It introduces a self-consistent calculation of all relevant corrections to helium-4 predictions, including correlations and detailed balance, and provides a computational tool for primordial abundance predictions.
Findings
Helium-4 mass fraction predicted as 0.24709±0.00017.
All corrections to weak interactions are included and verified for consistency.
The PRIMAT code enables precise primordial abundance calculations.
Abstract
Primordial nucleosynthesis is one of the three historical evidences for the big bang model, together with the expansion of the universe and the cosmic microwave background. Now that the number of neutrino families and the baryonic densities have been fixed by laboratory measurements or CMB observations, the model has no free parameter and its predictions are rigid. Departure from its predictions could provide hints or constraints on new physics or astrophysics in the early universe. Precision on primordial abundances deduced from observations have recently been drastically improved and reach the percent level for both deuterium and helium-4. Accordingly, the BBN predictions should reach the same level of precision. For most isotopes, the dominant sources of uncertainty come from those on the laboratory thermonuclear reactions. This article focuses on helium-4 whose predicted primordial…
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