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 Δα/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 Δα/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.
arXiv comment12 Pages, 7 figures. Accepted for publication in A&A. In addition to minor corrections an appendix is added in this revised version
References in corpus (15)
- Further Evidence for Cosmological Evolution of the Fine Structure Constant
- Further evidence for a variable fine-structure constant from Keck/HIRES QSO absorption spectra
- Limits on the time variation of the electromagnetic fine-structure constant in the low energy limit from absorption lines in the spectra of distant quasars
- Space-Time Variation of Physical Constants and Relativistic Corrections in Atoms
- Calculations of the Relativistic Effects in Many-Electron Atoms and Space-Time Variation of Fundamental Constants
- The VLT-UVES survey for molecular hydrogen in high-redshift damped Lyman-alpha systems
- Probing the cosmological variation of the fine-structure constant: Results based on VLT-UVES sample
- Probing the variability of the fine-structure constant with the VLT/UVES
- Astrophysical Limits on the Evolution of Dimensionless Physical Constants over Cosmological Time
- Further constraints on variation of the fine structure constant from alkali doublet QSO absorption lines
- Metals in the Intergalactic Medium
- Does the fine-structure constant vary with cosmological epoch?
- Constraining the variation of fundamental constants using 18cm OH lines
- Do the Fundamental Constants Vary in the Course of the Cosmological Evolution?
- Interferometric measurement of resonance transition wavelengths in C IV, Si IV, Al III, Al II, and Si II
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