Abstract
We determine the influence of a variation of the fundamental “constants” on the predicted helium abundance in Big Bang Nucleosynthesis. The analytic estimate is performed in two parts: the first step determines the dependence of the helium abundance on the nuclear physics parameters, while the second step relates those parameters to the fundamental couplings of particle physics. This procedure can incorporate in a flexible way the time variation of several couplings within a grand unified theory while keeping the nuclear physics computation separate from any GUT model dependence.
- Received 14 June 2004
DOI:https://doi.org/10.1103/PhysRevD.70.083504
©2004 American Physical Society