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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Published in | The European physical journal. A, Hadrons and nuclei Vol. 59; no. 10 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Berlin/Heidelberg
Springer Berlin Heidelberg
04.10.2023
|
Subjects | |
Online Access | Get full text |
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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. |
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ISSN: | 1434-601X 1434-601X |
DOI: | 10.1140/epja/s10050-023-01131-3 |