Probing the time-variation of the fine-structure constant: Results based on Si IV doublets from a UVES sample

dc.contributor.authorChand, Hum
dc.contributor.authorPetitjean, Patrick
dc.contributor.authorSrianand, R.
dc.contributor.authoret al.
dc.date.accessioned2012-03-07T10:58:42Z
dc.date.available2012-03-07T10:58:42Z
dc.date.issued2011-07-06
dc.description.abstractWe 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.urihttp://hdl.handle.net/11007/866
dc.language.isoenen_US
dc.relation.ispartofseriesIUCAA Preprints;34/04
dc.subjectQuasars: absorption linesen_US
dc.subjectCosmology: observationsen_US
dc.titleProbing the time-variation of the fine-structure constant: Results based on Si IV doublets from a UVES sampleen_US
dc.typeArticleen_US

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