Abstract
Observations of H2 spectra in the line-of-sight of distant quasars may reveal a variation of the proton-electron mass ratio μ = m p ∕ m e at high redshift, typically for z > 2. Currently four high-quality systems (Q0347-383, Q0405-443, Q0528-250 and J2123-050) have been analyzed returning a constraint Δμ ∕ μ < 1 ×10 − 5. We present data and a μ-variation analysis of another system, Q2348–011 at redshift z abs = 2. 42, delivering Δμ ∕ μ = ( − 1. 5 ± 1. 6) ×10 − 5. In addition to observational data the status of the laboratory measurements is reviewed. The future possibilities of deriving a competitive constraint on Δμ ∕ μ from the known high-redshift H2 absorbers is investigated, resulting in the identification of a number of potentially useful systems for detecting μ-variation.
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Acknowledgements
This work is based on observations carried out at the European Southern Observatory (ESO) under program ID 79.A-0404 (PI Ubachs), with the UVES spectrograph installed at the VLT Kueyen UT2 on Cerro Paranal, Chile. The authors wish to thank John Webb, Julian King and Steve Curran (Sydney), Adrian Malec (Melbourne) and Freek van Weerdenburg (Amsterdam) for fruitful discussions.
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Ubachs, W., Bagdonaite, J., Murphy, M.T., Buning, R., Kaper, L. (2011). Search for Cosmological μ-Variation from High-Redshift H2 Absorption; A Status Report. In: Martins, C., Molaro, P. (eds) From Varying Couplings to Fundamental Physics. Astrophysics and Space Science Proceedings. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-19397-2_13
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