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Indications of a Spatial Variation of the Fine Structure Constant | Phys. Rev. Lett.

    Indications of a Spatial Variation of the Fine Structure Constant

    J. K. Webb1, J. A. King1, M. T. Murphy2, V. V. Flambaum1, R. F. Carswell3, and M. B. Bainbridge1

    • 1School of Physics, University of New South Wales, Sydney, New South Wales 2052, Australia
    • 2Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Mail H30, PO Box 218, Victoria 3122, Australia
    • 3Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, United Kingdom

    Phys. Rev. Lett. 107, 191101 – Published 31 October, 2011

    DOI: https://doi.org/10.1103/PhysRevLett.107.191101

    Abstract

    We previously reported Keck telescope observations suggesting a smaller value of the fine structure constant α at high redshift. New Very Large Telescope (VLT) data, probing a different direction in the Universe, shows an inverse evolution; α increases at high redshift. Although the pattern could be due to as yet undetected systematic effects, with the systematics as presently understood the combined data set fits a spatial dipole, significant at the 4.2σ level, in the direction right ascension 17.5±0.9 h, declination 58±9 deg. The independent VLT and Keck samples give consistent dipole directions and amplitudes, as do high and low redshift samples. A search for systematics, using observations duplicated at both telescopes, reveals none so far which emulate this result.

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