VLT/UVES shows no cosmological variability of alpha
Abstract
The cosmological variability of alpha is probed from individual observations of pairs of FeII lines. This procedure allows a better control of the systematics and avoids the influence of the spectral shifts due to ionization inhomogeneities in the absorbers and/or non-zero offsets between different exposures. Applied to the FeII lines of the metal absorption systems at zabs = 1.839 in Q1101--264 and at zabs = 1.15 in HE0515--4414 observed by means of UVES at the ESO-VLT, it provides da/a = 0.4 (+/- 1.5 stat)x10^{-6}. The result is shifted with respect to the Keck/HIRES mean da/a = -5.7(+/- 1.1 stat})x10^{-6} (Murphy et al. 2004) at a high confidence level (95%). Full details of this work are given in Levshakov et al (2005)
Cite
@article{arxiv.astro-ph/0505090,
title = {VLT/UVES shows no cosmological variability of alpha},
author = {P. Molaro and M. Centurion and S. D'Odorico and S. Levshakov},
journal= {arXiv preprint arXiv:astro-ph/0505090},
year = {2009}
}
Comments
3 pages, 1 postscript figure