Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology · 2007 · 181 citations · 131 references
Natural SciencesPhysicsCosmologyNuclear PhysicsParticle PhysicsNuclear Binding EnergyNuclear Equation Of StateNuclear ModelsNuclear StructureNucleosynthesisStrong InteractionCouplingsDeuterium AbundanceFine Structure ConstantsNeutron Lifetime DiscrepancyNeutron Lifetime MeasurementNuclear CouplingPrimordial Nucleosynthesis ConstraintsYukawa Potential
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 $^{4}\mathrm{He}$, 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 $^{7}\mathrm{Li}$ abundance deduced from the WMAP analysis with its spectroscopically determined value while maintaining concordance with D and $^{4}\mathrm{He}$. 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 $\ensuremath{\sigma}$ and $\ensuremath{\omega}$ 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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The Ame2003 atomic mass evaluation
G. Audi, A.H. Wapstra, C. Thibault · Nuclear Physics A · 2003 · 4.8K citations
Journal of Physics G Nuclear and Particle Physics · 2006 · 4.1K citations · Full text
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Upper bounds on supersymmetric particle masses
Riccardo Barbieri, Gian F. Giudice · Nuclear Physics B · 1988 · 1.1K citations · Full text
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