STScI Preprint #1284
We discuss how laboratory experiments can be used to place constraints on possible variations of the fine structure constant in the observationally relevant redshift interval z
0 - 5, within a rather general theoretical framework. We find a worst case upper limit for
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of 8 × 10-6 for z
5 and
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of 0.9 × 10-6 for z
1.6. The derived limits are at variance with the recent findings by Webb et al. (1998), who claim an observed variation of
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= -2.6 ± 0.4 × 10-5 at 1<z<1.6.
1) Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
2) On leave from the Scuola Normale Superiore, Piazza dei Cavalieri 7, I56126 Pisa, Italy
3) On assignment from the Space Science Dept. of the European Space Agency