Primordial Helium Production in a Charged Universe
  We use the constraints arising from primordial nucleosynthesis to bound a putative electric charge density $|e|n_q$ of the universe. We find $|n_q/n_\gamma| \lesssim 10^{-43}$, four orders of magnitude more stringent than previous limits. We also work out the bounds on $n_q$ in models with a photon mass, that allows to have a charge density without large-scale electric fields. 
Eduard Masso (UAB, Barcelona) and Francesc Rota (UAB, Barcelona)