A new measure of Delta alpha/alpha at redshift z = 1.84 from very high resolution spectra of Q1101-264
arXiv:astro-ph/0703042 · doi:10.1051/0004-6361:20066064
Abstract
We probe the evolution of the fine-structure constant, alpha, with cosmic time. Accurate positions of the FeII lines 1608, 2382,and 2600 A are measured in the z = 1.84 absorption system from a high-resolution (FWHM = 3.8 km/s) and high signal-to-noise (S/N >= 100) spectrum of the quasar Q1101-264 (z_em = 2.15, V = 16.0), integrated for 15.4 hours. The Single Ion Differential alpha Measurement (SIDAM) procedure and the Delta chi^2 method are used to set constraints on Delta alpha/alpha. We have found a relative radial velocity shift between the 1608 A and 2382,2600 A lines of Delta v = -180 +/- 85 m/s (both random and systematic errors are included), which, if real, would correspond to Delta alpha/alpha = (5.4 +/- 2.5) 10^{-6} (1sigma C.L.). Considering the strong implications of a such variability, additional observations with comparable accuracy at redshift z ~ 1.8 are required to confirm this result.
8 pages, 5 figures, accepted for publication as a research note in A&A
References in corpus (5)
- Dynamics of dark energy
- Limit on the Temporal Variation of the Fine-Structure Constant Using Atomic Dysprosium
- Time-variability of alpha from realistic models of Oklo reactors
- Reconstructing the dark energy equation of state with varying couplings
- Accurate laboratory ultraviolet wavelengths for quasar absorption-line constraints on varying fundamental constants
Cited by in corpus (26)
- Enhanced sensitivity to variation of the fine structure constant and m_p/m_e in diatomic molecules
- Impact of instrumental systematic errors on fine-structure constant measurements with quasar spectra
- Revision of VLT/UVES constraints on a varying fine-structure constant
- UVES radial velocity accuracy from asteroid observations. Implications for the fine structure constant variability
- High-precision limit on variation in the fine-structure constant from a single quasar absorption system
- The UVES Large Program for testing fundamental physics - III. Constraints on the fine-structure constant from 3 telescopes
- Bounds on the fine structure constant variability from FeII absorption lines in QSO spectra
- Subaru Telescope limits on cosmological variations in the fine-structure constant
- Fundamental physics with ESPRESSO: Precise limit on variations in the fine-structure constant towards the bright quasar HE 05154414
- Is there further evidence for spatial variation of fundamental constants?
- Fundamental physics with Espresso: Towards an accurate wavelength calibration for a precision test of the fine-structure constant
- -doublet spectra of diatomic radicals and their dependence on fundamental constants
- A new approach for testing variations of fundamental constants over cosmic epochs using FIR fine-structure lines
- Isotope shift calculations in Ti II
- Transition frequency shifts with fine structure constant variation for Fe II: Breit and core-valence correlation correction
- Variability of the proton-to-electron mass ratio on cosmological scales
- Varying couplings in the early universe: correlated variations of and
- Transition frequency shifts with fine-structure constant variation for Fe I. Isotope shift calculations in Fe I and Fe II
- Cosmological Evolution of Fundamental Constants: From Theory to Experiment
- Mid- and far-infrared fine-structure line sensitivities to hypothetical variability of the fine-structure constant
- Dark energy constraints from ESPRESSO tests of the stability of fundamental couplings
- Redshifting of cosmological black bodies in BSBM varying-alpha theories
- Possible time-variability of the fine-structure constant expected from the accelerating universe
- Sensitivity coefficients to -variation for fine-structure transitions in Carbon-like ions
- The time variation of the fine structure constant: A statistical analysis of astronomical data
- Sensitivity coefficients to -variation for astrophysically relevant transitions in Ni II