alpha
We have put constraints on the variation of the fine structure constant, $\alpha$, using recent Cosmic Microwave Background, CMB, observations.
This study gave rise to the following papers:
Last updated: 2004 August. The astro-ph archive can be searched for an up to date lists of my papers: for au=G. Rocha and ti=alpha which gives an incomplete list, to be completed with au=G. Rocha and ti=fine structure constant
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