arXiv · 0711.4055
Phase transition in the fine structure constant
Abstract
Within the context of mass-varying neutrinos, we construct a cosmological model that has a phase transition in the electromagnetic fine structure constant αat a redshift of 0.5. The model accommodates hints of a time variable αin quasar spectra and the nonobservance of such an effect at very low redshifts. It is consistent with limits from the recombination and primordial nucleosynthesis eras and is free of instabilities.
Explore related subjects
Keep this discovery
L. Anchordoqui, V. Barger, H. Goldberg, D. Marfatia. 2008-01-25. Phase transition in the fine structure constant. https://doi.org/10.1016/j.physletb.2008.01.047
Cite the original work for its findings. Save a collection to share your selection of sources.