Journal Article

Constraining the variation of fundamental constants at <i>z</i> ∼ 1.3 using 21-cm absorbers<sup>⋆</sup>

H. Rahmani, R. Srianand, N. Gupta, P. Petitjean, P. Noterdaeme and D. Albornoz Vásquez

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 425, issue 1, pages 556-576
Published in print September 2012 | ISSN: 0035-8711
Published online September 2012 | e-ISSN: 1365-2966 | DOI:
Constraining the variation of fundamental constants at z ∼ 1.3 using 21-cm absorbers⋆

More Like This

Show all results sharing this subject:

  • Astronomy and Astrophysics


Show Summary Details



We present high-resolution optical spectra obtained with the Ultraviolet and Visual Echelle Spectrograph at the Very Large Telescope and 21-cm absorption spectra obtained with the Giant Metrewave Radio Telescope and the Green Bank Telescope of five quasars along the line of sight of which 21-cm absorption systems at 1.17 < z < 1.56 have been detected previously. We also present milliarcsecond-scale radio images of these quasars obtained with the Very Large Baseline Array. We use the data on four of these systems to constrain the time variation of xgpα2/μ, where gp is the proton gyromagnetic factor, α is the fine structure constant and μ is the proton-to-electron mass ratio. We carefully evaluate the systematic uncertainties in redshift measurements using cross-correlation analysis and repeated Voigt profile fitting. In both cases, we also confirm our results by analysing optical spectra obtained with the Keck telescope. We find the weighted and the simple means of Δx/x to be, respectively, −(0.1 ± 1.3) × 10−6 and (0.0 ± 1.5) × 10−6 at the mean redshift of 〈z〉 = 1.36 corresponding to a look-back time of ∼9 Gyr. This is the most stringent constraint ever obtained on Δx/x. If we only use the two systems towards quasars unresolved at milliarcsecond scales, we get the simple mean of Δx/x = +(0.2 ± 1.6) × 10−6. Assuming the constancy of other constants, we get Δα/α = (0.0 ± 0.8) × 10−6, which is a factor of 2 better than the best constraints obtained so far using the many-multiplet method. On the other hand, assuming that α and gp have not varied we derive Δμ/μ = (0.0 ± 1.5) × 10−6 which is again the best limit ever obtained on the variation of μ over this redshift range. Using independent constraints on Δα/α at z < 1.8 and Δμ/μ at z ∼ 0.7 available in the literature, we get Δgp/gp ≤ 3.5 × 10−6(1σ).

Keywords: quasars: absorption lines; quasars: individual: J0108−0037; quasars: individual: J0501−0159; quasars: individual: J1623+0718; quasars: individual: J2340−0053; quasars: individual: J2358−1020

Journal Article.  11322 words.  Illustrated.

Subjects: Astronomy and Astrophysics

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.