Probing the time-variation of the fine-structure constant: Results based on Si IV doublets from a UVES sample
| dc.contributor.author | Chand, Hum | |
| dc.contributor.author | Petitjean, Patrick | |
| dc.contributor.author | Srianand, R. | |
| dc.contributor.author | et al. | |
| dc.date.accessioned | 2012-03-07T10:58:42Z | |
| dc.date.available | 2012-03-07T10:58:42Z | |
| dc.date.issued | 2011-07-06 | |
| dc.description.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 ∆α/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 ∆α/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. | en_US |
| dc.identifier.uri | http://hdl.handle.net/11007/866 | |
| dc.language.iso | en | en_US |
| dc.relation.ispartofseries | IUCAA Preprints;34/04 | |
| dc.subject | Quasars: absorption lines | en_US |
| dc.subject | Cosmology: observations | en_US |
| dc.title | Probing the time-variation of the fine-structure constant: Results based on Si IV doublets from a UVES sample | en_US |
| dc.type | Article | en_US |