Abstract (EN):
We examine the variation of the fine structure constant in the context of a two-field quintessence model. We find that, for solutions that lead to a transient late period of accelerated expansion, it is possible to fit the data arising from quasar spectra and comply with the bounds on the variation of alpha from the Oklo reactor, meteorite analysis, atomic clock measurements, cosmic microwave background radiation, and big bang nucleosynthesis. That is more difficult if we consider solutions corresponding to a late period of permanent accelerated expansion.
Language:
English
Type (Professor's evaluation):
Scientific
Contact:
bento@sirius.ist.utl.pt; orfeu@cosmos.ist.utl.pt; ncsantos@cfif.ist.utl.pt
No. of pages:
4