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arxiv: astro-ph/0610733 · v2 · submitted 2006-10-24 · 🌌 astro-ph

Coupled Variations of Fundamental Couplings and Primordial Nucleosynthesis

classification 🌌 astro-ph
keywords constraintsfundamentalvariationanalysisbindingcouplingsenergymass
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The effect of variations of the fundamental nuclear parameters on big-bang nucleosynthesis are modeled and discussed in detail taking into account the interrelations between the fundamental parameters arising in unified theories. Considering only \he4, strong constraints on the variation of the neutron lifetime, neutron-proton mass difference are set. These constraints are then translated into constraints on the time variation of the Yukawa couplings and the fine structure constant. Furthermore, we show that a variation of the deuterium binding energy is able to reconcile the \li7 abundance deduced from the WMAP analysis with its spectroscopically determined value while maintaining concordance with D and \he4. The analysis is strongly based on the potential model of Flambaum and Shuryak that relates the binding energy of the deuteron with the nucleon and $\sigma$ and $\omega$ mesons masses, however, we show that an alternative approach that consists of a pion mass dependence necessarily leads to equivalent conclusions.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Probing Unification Scenarios with Big Bang Nucleosynthesis

    hep-ph 2026-04 unverdicted novelty 4.0

    Extending a BBN code yields constraints Δα/α = 2 ± 51 ppm (mass variation) and 2 ± 22 ppm (G variation) at 68% CL, showing these models do not solve the lithium problem.

  2. Fine-tunings in radiative $\alpha$-particle capture on $^{12}$C at astrophysical energies

    nucl-th 2026-01 unverdicted novelty 4.0

    Astrophysical S-factor data constrain variations in the electromagnetic fine-structure constant to |δ α/α| ≤ 0.0002 in radiative alpha capture on carbon-12.