English

Probing Unification Scenarios with Big Bang Nucleosynthesis

High Energy Physics - Phenomenology 2026-04-07 v1 Cosmology and Nongalactic Astrophysics

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, α\alpha, 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 68%68\% confidence level a constraint on the relative variation of α\alpha, between the BBN epoch and the present-day laboratory value, of Δα/α=2±51\Delta\alpha/\alpha=2\pm51 ppm (parts per million), while for the variation of Newton's constant the analogous constraint is Δα/α=2±22\Delta\alpha/\alpha=2\pm22 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)