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 Δα/α = (+0.15 ± 0.43) × 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 Δα/α based 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.
CITATION STYLE
Chand, H., Petitjean, P., Srianand, R., & Aracil, B. (2005). Probing the time-variation of the fine-structure constant: Results based on SI IV doublets from a UVES sample. Astronomy and Astrophysics, 430(1), 47–58. https://doi.org/10.1051/0004-6361:20041186
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