Probing Unification Scenarios with Big Bang Nucleosynthesis
Abstract
We extend a recently developed Big Bang Nucleosynthesis (BBN) code, {\tt PRyMordial}, to constrain a broad class of Grand Unified Theories to which BBN is sensitive, since these lead to varying fundamental couplings. A previously developed self-consistent perturbative analysis of the effects of these variations has been implemented in {\tt PRyMordial}, leading to robust constraints of the value of the fine-structure constant, , at the BBN epoch using current observations of Helium-4 and Deuterium abundances. We explored two different viable scenarios, relying on alternative assumptions on the gravitational sector: the variation of the gravitational coupling can be implemented by varying either particle masses, or Newton's gravitational constant. For the variation of masses, we obtained at confidence level a constraint on the relative variation of , between the BBN epoch and the present-day laboratory value, of ppm (parts per million), while for the variation of Newton's constant the analogous constraint is ppm. We also show that, given these constraints, these models do not provide a solution to the cosmological Lithium problem.
Keywords
Cite
@article{arxiv.2604.04870,
title = {Probing Unification Scenarios with Big Bang Nucleosynthesis},
author = {I. M. Dreyer and C. J. A. P. Martins},
journal= {arXiv preprint arXiv:2604.04870},
year = {2026}
}
Comments
12 pages, 11 figures 1 table; Phys. Rev. D (in press)