EDP Sciences
Free Access
Issue
A&A
Volume 440, Number 1, September II 2005
Page(s) 45 - 52
Section Cosmology (including clusters of galaxies)
DOI https://doi.org/10.1051/0004-6361:20052648
Published online 19 August 2005


A&A 440, 45-52 (2005)
DOI: 10.1051/0004-6361:20052648

A new constraint on the time dependence of the proton-to-electron mass ratio

Analysis of the Q 0347-383 and Q 0405-443 spectra
A. Ivanchik1, P. Petitjean2, 3, D. Varshalovich1, B. Aracil2, 4, R. Srianand5, H. Chand5, C. Ledoux6 and P. Boissé2, 3

1  Ioffe Physical Technical Institute, Polytekhnicheskaya 26, 194021 Saint-Petersburg, Russia
    e-mail: iav@astro.ioffe.rssi.ru
2  Institut d'Astrophysique de Paris - CNRS, 98bis Boulevard Arago, 75014 Paris, France
    e-mail: ppetitje@iap.fr
3  LERMA, Observatoire de Paris, 61 avenue de l'Observatoire, 75014 Paris, France
4  Department of Astronomy, University of Massachusetts, 710 North Pleasant Street, Amherst, MA 01003-9305, USA
5  IUCAA, Post Bag 4, Ganeshkhind, Pune 411007, India
6  European Southern Observatory, Alonso de Córdova 3107, Casilla 19001, Vitacura, Santiago, Chile

(Received 2 January 2004 / Accepted 10 May 2005)

Abstract
A new limit on the possible cosmological variation of the proton-to-electron mass ratio $\mu=m_{\rm p}/m_{\rm e}$ is estimated by measuring wavelengths of H2 lines of Lyman and Werner bands from two absorption systems at $z_{\rm abs}=2.5947$ and 3.0249 in the spectra of quasars Q 0405-443 and Q 0347-383, respectively. Data are of the highest spectral resolution (R = 53 000) and S/N ratio (30$\div$70) for this kind of study. We search for any correlation between $z_{\rm i}$, the redshift of observed lines, determined using laboratory wavelengths as references, and $K_{\rm i}$, the sensitivity coefficient of the lines to a change of $\mu$, that could be interpreted as a variation of $\mu$ over the corresponding cosmological time. We use two sets of laboratory wavelengths, the first one, Set (A) (Abgrall et al. 1993, J. Mol. Spec., 157, 512), based on experimental determination of energy levels and the second one, Set (P) (Philip et al. 2004, Can. J. Chem., 82, 713), based on new laboratory measurements of some individual rest-wavelengths. We find $\Delta\mu$/$\mu$ = (3.05 $\pm$ 0.75) $\times$ 10-5 for Set (A), and $\Delta\mu$/$\mu$ = (1.65 $\pm$ 0.74) $\times$ 10-5 for Set (P). The second determination is the most stringent limit on the variation of $\mu$ over the last 12 Gyr ever obtained. The correlation found using Set (A) seems to show that some amount of systematic error is hidden in the determination of energy levels of the H2 molecule.


Key words: cosmology: theory -- cosmology: observations -- quasars: absorption lines -- quasars: individual: Q 0405-443 -- quasars: individual: Q 0347-383

SIMBAD Objects



© ESO 2005

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