Probing the time-variation of the fine-structure constant: Results based on Si IV doublets from a UVES sample
arXiv:astro-ph/0408200 · doi:10.1051/0004-6361:20041186
Abstract
We report a new constraint on the variation of the fine-structure constant based on the analysis of 15 Si IV doublets selected from a ESO-UVES sample. We find Îα/α= (+0.15+/-0.43) x 10^-5 over a redshift range of 1.59< z < 2.92 which is consistent with no variation in α. This result represents a factor of three improvement on the constraint on Îα/αbased on Si IV doublets compared to the published results in the literature. The alkali doublet method used here avoids the implicit assumptions used in the many-multiplet method that chemical and ionization inhomogeneities are negligible and isotopic abundances are close to the terrestrial value.
12 Pages, 7 figures. Accepted for publication in A&A. In addition to minor corrections an appendix is added in this revised version