The electromagnetic fine-structure constant in primordial nucleosynthesis revisited

We study the dependence of the primordial nuclear abundances as a function of the electromagnetic fine-structure constant α , keeping all other fundamental constants fixed. We update the leading nuclear reaction rates, in particular the electromagnetic contribution to the neutron-proton mass differe...

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Bibliographic Details
Published inThe European physical journal. A, Hadrons and nuclei Vol. 59; no. 10
Main Authors Meißner, Ulf-G., Metsch, Bernard Ch, Meyer, Helen
Format Journal Article
LanguageEnglish
Published Berlin/Heidelberg Springer Berlin Heidelberg 04.10.2023
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Summary:We study the dependence of the primordial nuclear abundances as a function of the electromagnetic fine-structure constant α , keeping all other fundamental constants fixed. We update the leading nuclear reaction rates, in particular the electromagnetic contribution to the neutron-proton mass difference pertinent to β -decays, and go beyond certain approximations made in the literature. In particular, we include the temperature-dependence of the leading nuclear reactions rates and assess the systematic uncertainties by using four different publicly available codes for Big Bang nucleosynthesis. Disregarding the unsolved so-called lithium-problem, we find that the current values for the observationally based 2 H and 4 He abundances restrict the fractional change in the fine-structure constant to less than 2 %  , which is a tighter bound than found in earlier works on the subject.
ISSN:1434-601X
1434-601X
DOI:10.1140/epja/s10050-023-01131-3