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A molecular probe of dark energy
Authors:Rodger I. Thompson  Jill Bechtold  Daniel Eisenstein  Xiaohui Fan  David Arnett  Carlos Martins  Robert Kennicutt  John Black
Affiliation:1. Steward Observatory, University of Arizona, Tucson, AZ 85721, USA;2. University of Cambridge, Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK;3. Centro de Fisica do Porto, Rua das Estrelas sn, 4150-762 Porto, Portugal;4. Chalmers University, Onsala Space Observatory, SE-43992 Onsala, Sweden
Abstract:Many theoretical models of dark energy invoke rolling scaler fields which in turn predict time varying values of the fundamental constants. Establishing the value of the fundamental constants at various times in the universe can probe and test the various dark energy theories. One of the constants that is predicted to vary is the ratio of the electron to proton mass μ. It was established early on that molecular spectra are sensitive to the value of μ and can be used as probes of that value. This article describes the use of the spectrum of molecular hydrogen in high redshift Damped Lyman Alpha systems (DLAs) as a sensitive probe of the time evolution of μ.
Keywords:Dark energy
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